Abel, T. and Wandelt, B. D. (2002). Adaptive ray tracing for radiative transfer around point sources. MNRAS, 330:L53–L56.
Agertz, O. and Kravtsov, A. V. (2015). On the Interplay between Star Formation and Feedback in Galaxy Formation Simulations. ApJ, 804:18.
Agertz, O., Kravtsov, A. V., Leitner, S. N., and Gnedin, N. Y. (2013). Toward a Complete Accounting of Energy and Momentum from Stellar Feedback in Galaxy Formation Simulations. ApJ, 770:25.
Agertz, O., Moore, B., Stadel, J., Potter, D., Miniati, F., Read, J., Mayer, L., Gawryszczak, A., Kravtsov, A., Nordlund, Å., Pearce, F., Quilis, V., Rudd, D., Springel, V., Stone, J., Tasker, E., Teyssier, R., Wadsley, J., and Walder, R. (2007). Fundamental differences between SPH and grid methods. MNRAS, 380:963–978.
Agertz, O., Teyssier, R., and Moore, B. (2011). The formation of disc galaxies in a ΛCDM universe. MNRAS, 410:1391–1408.
Altay, G., Croft, R. A. C., and Pelupessy, I. (2008). SPHRAY: a smoothed particle hydrodynamics ray tracer for radiative transfer. MNRAS, 386:1931–1946.
Arthur, S. J. (2012). What produces the diffuse X-ray emission from the Orion nebula? I. Simple spherical models. MNRAS, 421:1283–1297.
Arthur, S. J., Henney, W. J., Mellema, G., de Colle, F., and Vázquez-Semadeni, E. (2011). Radiation-magnetohydrodynamic simulations of H II regions and their associated PDRs in turbulent molecular clouds. MNRAS, 414:1747–1768.
Arthur, S. J. and Hoare, M. G. (2006). Hydrodynamics of Cometary Compact H II Regions. ApJS, 165:283–306.
Aumer, M., White, S. D. M., Naab, T., and Scannapieco, C. (2013). Towards a more realistic population of bright spiral galaxies in cosmological simulations. MNRAS, 434:3142–3164.
Balick, B. and Frank, A. (2002). Shapes and Shaping of Planetary Nebulae. ARA&A, 40:439–486.
Banerjee, R., Klessen, R. S., and Fendt, C. (2007). Can Protostellar Jets Drive Supersonic Turbulence in Molecular Clouds? ApJ, 668:1028–1041.
Bate, M. R. (2009). The importance of radiative feedback for the stellar initial mass function. MNRAS, 392:1363–1380.
Bate, M. R. (2014). The statistical properties of stars and their dependence on metallicity: the effects of opacity. MNRAS, 442:285–313.
Bate, M. R., Bonnell, I. A., and Price, N. M. (1995). Modelling accretion in protobinary systems. MNRAS, 277:362–376.
Bate, M. R. and Keto, E. R. (2015). Combining radiative transfer and diffuse interstellar medium physics to model star formation. MNRAS, 449:2643–2667.
Bertoldi, F. (1989). The photoevaporation of interstellar clouds. I - Radiation-driven implosion. ApJ, 346:735–755.
Bisbas, T. G., Wünsch, R., Whitworth, A. P., and Hubber, D. A. (2009). Smoothed particle hydrodynamics simulations of expanding H II regions. I. Numerical method and applications. A&A, 497:649–659.
Bisbas, T. G., Wünsch, R., Whitworth, A. P., Hubber, D. A., and Walch, S. (2011). Radiation-driven Implosion and Triggered Star Formation. ApJ, 736:142.
Bodenheimer, P., Laughlin, G. P., Rózyczka, M., and Yorke, H. W., editors (2007). Numerical Methods in Astrophysics: An Introduction.
Boneberg, D. M., Dale, J. E., Girichidis, P., and Ercolano, B. (2015). Turbulence in giant molecular clouds: the effect of photoionization feedback. MNRAS, 447:1341–1352.
Bonnell, I. A., Dobbs, C. L., and Smith, R. J. (2013). Shocks, cooling and the origin of star formation rates in spiral galaxies. MNRAS, 430:1790–1800.
Brook, C. B., Stinson, G., Gibson, B. K., Wadsley, J., and Quinn, T. (2012). MaGICC discs: matching observed galaxy relationships over a wide stellar mass range. MNRAS, 424:1275–1283.
Capriotti, E. R. and Kozminski, J. F. (2001). Relative Effects of Ionizing Radiation and Winds from O-Type Stars on the Structure and Dynamics of H II Regions. PASP, 113:677–691.
Carroll, J. J., Frank, A., Blackman, E. G., Cunningham, A. J., and Quillen, A. C. (2009). Outflow-Driven Turbulence in Molecular Clouds. ApJ, 695:1376–1381.
Castor, J., McCray, R., and Weaver, R. (1975). Interstellar bubbles. ApJL, 200:L107–L110.
Ceverino, D., Klypin, A., Klimek, E. S., Trujillo-Gomez, S., Churchill, C. W., Primack, J., and Dekel, A. (2014). Radiative feedback and the low efficiency of galaxy formation in low-mass haloes at high redshift. MNRAS, 442:1545–1559.
Clark, P. C. and Glover, S. C. O. (2014). On column density thresholds and the star formation rate. MNRAS, 444:2396–2414.
Clark, P. C., Glover, S. C. O., and Klessen, R. S. (2012a). TreeCol: a novel approach to estimating column densities in astrophysical simulations. MNRAS, 420:745–756.
Clark, P. C., Glover, S. C. O., Klessen, R. S., and Bonnell, I. A. (2012b). How long does it take to form a molecular cloud? MNRAS, 424:2599–2613.
Clark, P. C., Glover, S. C. O., Smith, R. J., Greif, T. H., Klessen, R. S., and Bromm, V. (2011). The Formation and Fragmentation of Disks Around Primordial Protostars. Science, 331:1040–.
Colín, P., Vázquez-Semadeni, E., and Gómez, G. C. (2013). Molecular cloud evolution - V. Cloud destruction by stellar feedback. MNRAS, 435:1701–1714.
Crain, R. A., Schaye, J., Bower, R. G., Furlong, M., Schaller, M., Theuns, T., Dalla Vecchia, C., Frenk, C. S., McCarthy, I. G., Helly, J. C., Jenkins, A., Rosas-Guevara, Y. M., White, S. D. M., and Trayford, J. W. (2015). The EAGLE simulations of galaxy formation: calibration of subgrid physics and model variations. MNRAS, 450:1937–1961.
Cunningham, A. J., Klein, R. I., Krumholz, M. R., and McKee, C. F. (2011). Radiation-hydrodynamic Simulations of Massive Star Formation with Protostellar Outflows. ApJ, 740:107.
Dale, J. E. and Bonnell, I. (2011). Ionizing feedback from massive stars in massive clusters: fake bubbles and untriggered star formation. MNRAS, 414:321–328.
Dale, J. E. and Bonnell, I. A. (2008). The effect of stellar winds on the formation of a protocluster. MNRAS, 391:2–13.
Dale, J. E. and Bonnell, I. A. (2012). Ionization-induced star formation - III. Effects of external triggering on the initial mass function in clusters. MNRAS, 422:1352–1362.
Dale, J. E., Bonnell, I. A., Clarke, C. J., and Bate, M. R. (2005). Photoionizing feedback in star cluster formation. MNRAS, 358:291–304.
Dale, J. E., Bonnell, I. A., and Whitworth, A. P. (2007a). Ionization-induced star formation - I. The collect-and-collapse model. MNRAS, 375:1291–1298.
Dale, J. E., Clark, P. C., and Bonnell, I. A. (2007b). Ionization-induced star formation - II. External irradiation of a turbulent molecular cloud. MNRAS, 377:535–544.
Dale, J. E., Ercolano, B., and Bonnell, I. A. (2012a). Ionization-induced star formation - IV. Triggering in bound clusters. MNRAS, 427:2852–2865.
Dale, J. E., Ercolano, B., and Bonnell, I. A. (2012b). Ionizing feedback from massive stars in massive clusters - II. Disruption of bound clusters by photoionization. MNRAS, 424:377–392.
Dale, J. E., Ercolano, B., and Bonnell, I. A. (2013a). Ionization-induced star formation - V. Triggering in partially unbound clusters. MNRAS, 431:1062–1076.
Dale, J. E., Ercolano, B., and Bonnell, I. A. (2013b). Ionizing feedback from massive stars in massive clusters - III. Disruption of partially unbound clouds. MNRAS, 430:234–246.
Dale, J. E., Ercolano, B., and Clarke, C. J. (2007c). A new algorithm for modelling photoionizing radiation in smoothed particle hydrodynamics. MNRAS, 382:1759–1767.
Dale, J. E., Haworth, T. J., and Bressert, E. (2015). The dangers of being trigger-happy. MNRAS, 450:1199–1211.
Dale, J. E., Ngoumou, J., Ercolano, B., and Bonnell, I. A. (2013c). Massive stars in massive clusters - IV. Disruption of clouds by momentum-driven winds. MNRAS, 436:3430–3445.
Dale, J. E., Ngoumou, J., Ercolano, B., and Bonnell, I. A. (2014). Before the first supernova: combined effects of H II regions and winds on molecular clouds. MNRAS, 442:694–712.
Davis, S. W., Jiang, Y.-F., Stone, J. M., and Murray, N. (2014). Radiation Feedback in ULIRGs: Are Photons Movers and Shakers? ApJ, 796:107.
Davis, S. W., Stone, J. M., and Jiang, Y.-F. (2012). A Radiation Transfer Solver for Athena Using Short Characteristics. ApJS, 199:9.
Dobbs, C. L. (2015). The interstellar medium and star formation on kpc size scales. MNRAS, 447:3390–3401.
Dobbs, C. L., Burkert, A., and Pringle, J. E. (2011). The properties of the interstellar medium in disc galaxies with stellar feedback. MNRAS, 417:1318–1334.
Dobbs, C. L. and Pringle, J. E. (2013). The exciting lives of giant molecular clouds. MNRAS, 432:653–667.
Dubois, Y. and Teyssier, R. (2008). On the onset of galactic winds in quiescent star forming galaxies. A&A, 477:79–94.
Durier, F. and Dalla Vecchia, C. (2012). Implementation of feedback in smoothed particle hydrodynamics: towards concordance of methods. MNRAS, 419:465–478.
Elmegreen, B. G. and Elmegreen, D. M. (1978). Star formation in shock-compressed layers. ApJ, 220:1051–1062.
Ercolano, B., Barlow, M. J., Storey, P. J., and Liu, X.-W. (2003). MOCASSIN: a fully three-dimensional Monte Carlo photoionization code. MNRAS, 340:1136–1152.
Fabian, A. C. (2012). Observational Evidence of Active Galactic Nuclei Feedback. ARA&A, 50:455–489.
Fall, S. M., Krumholz, M. R., and Matzner, C. D. (2010). Stellar Feedback in Molecular Clouds and its Influence on the Mass Function of Young Star Clusters. ApJL, 710:L142–L146.
Federrath, C., Banerjee, R., Clark, P. C., and Klessen, R. S. (2010). Modeling Collapse and Accretion in Turbulent Gas Clouds: Implementation and Comparison of Sink Particles in AMR and SPH. ApJ, 713:269–290.
Federrath, C., Schrön, M., Banerjee, R., and Klessen, R. S. (2014). Modeling Jet and Outflow Feedback during Star Cluster Formation. ApJ, 790:128.
Ferland, G. J., Korista, K. T., Verner, D. A., Ferguson, J. W., Kingdon, J. B., and Verner, E. M. (1998). CLOUDY 90: Numerical Simulation of Plasmas and Their Spectra. PASP, 110:761–778.
Franco, J., Tenorio-Tagle, G., and Bodenheimer, P. (1990). On the formation and expansion of H II regions. ApJ, 349:126–140.
Frank, A., Ray, T. P., Cabrit, S., Hartigan, P., Arce, H. G., Bacciotti, F., Bally, J., Benisty, M., Eislöffel, J., Güdel, M., Lebedev, S., Nisini, B., and Raga, A. (2014). Jets and Outflows from Star to Cloud: Observations Confront Theory. Protostars and Planets VI, pages 451–474.
Freyer, T., Hensler, G., and Yorke, H. W. (2003). Massive Stars and the Energy Balance of the Interstellar Medium. I. The Impact of an Isolated 60 solar mass Star. ApJ, 594:888–910.
Freyer, T., Hensler, G., and Yorke, H. W. (2006). Massive Stars and the Energy Balance of the Interstellar Medium. II. The 35 solar mass Star and a Solution to the “Missing Wind Problem”. ApJ, 638:262–280.
Fryxell, B., Olson, K., Ricker, P., Timmes, F. X., Zingale, M., Lamb, D. Q., MacNeice, P., Rosner, R., Truran, J. W., and Tufo, H. (2000). FLASH: An Adaptive Mesh Hydrodynamics Code for Modeling Astrophysical Thermonuclear Flashes. ApJS, 131:273–334.
Furukawa, N., Dawson, J. R., Ohama, A., Kawamura, A., Mizuno, N., Onishi, T., and Fukui, Y. (2009). Molecular Clouds Toward RCW49 and Westerlund 2: Evidence for Cluster Formation Triggered by Cloud-Cloud Collision. ApJL, 696:L115–L119.
Gaburov, E. and Nitadori, K. (2011). Astrophysical weighted particle magnetohydrodynamics. MNRAS, 414:129–154.
Garcia-Segura, G. and Franco, J. (1996). From Ultracompact to Extended H II Regions. ApJ, 469:171.
Gatto, A., Walch, S., Low, M.-M. M., Naab, T., Girichidis, P., Glover, S. C. O., Wünsch, R., Klessen, R. S., Clark, P. C., Baczynski, C., Peters, T., Ostriker, J. P., Ibáñez-Mejía, J. C., and Haid, S. (2015). Modelling the supernova-driven ISM in different environments. MNRAS, 449:1057–1075.
Gendelev, L. and Krumholz, M. R. (2012). Evolution of Blister-type H II Regions in a Magnetized Medium. ApJ, 745:158.
Genzel, R., Newman, S., Jones, T., Förster Schreiber, N. M., Shapiro, K., Genel, S., Lilly, S. J., Renzini, A., Tacconi, L. J., Bouché, N., Burkert, A., Cresci, G., Buschkamp, P., Carollo, C. M., Ceverino, D., Davies, R., Dekel, A., Eisenhauer, F., Hicks, E., Kurk, J., Lutz, D., Mancini, C., Naab, T., Peng, Y., Sternberg, A., Vergani, D., and Zamorani, G. (2011). The Sins Survey of z ~ 2 Galaxy Kinematics: Properties of the Giant Star-forming Clumps. ApJ, 733:101.
Giuliani, Jr., J. L. (1979). The hydrodynamic stability of ionization-shock fronts - Linear theory. ApJ, 233:280–293.
Glover, S. C. O. and Clark, P. C. (2012a). Approximations for modelling CO chemistry in giant molecular clouds: a comparison of approaches. MNRAS, 421:116–131.
Glover, S. C. O. and Clark, P. C. (2012b). Is molecular gas necessary for star formation? MNRAS, 421:9–19.
Glover, S. C. O. and Mac Low, M.-M. (2007). Simulating the Formation of Molecular Clouds. II. Rapid Formation from Turbulent Initial Conditions. ApJ, 659:1317–1337.
Gnedin, N. Y. and Abel, T. (2001). Multi-dimensional cosmological radiative transfer with a Variable Eddington Tensor formalism. NewA, 6:437–455.
Górski, K. M., Hivon, E., Banday, A. J., Wandelt, B. D., Hansen, F. K., Reinecke, M., and Bartelmann, M. (2005). HEALPix: A Framework for High-Resolution Discretization and Fast Analysis of Data Distributed on the Sphere. ApJ, 622:759–771.
Greif, T. H. (2015). The numerical frontier of the high-redshift Universe. Computational Astrophysics and Cosmology, 2:3.
Gritschneder, M., Burkert, A., Naab, T., and Walch, S. (2010). Detailed Numerical Simulations on the Formation of Pillars Around H II Regions. ApJ, 723:971–984.
Gritschneder, M., Naab, T., Burkert, A., Walch, S., Heitsch, F., and Wetzstein, M. (2009a). iVINE - Ionization in the parallel TREE/SPH code VINE: first results on the observed age-spread around O-stars. MNRAS, 393:21–31.
Gritschneder, M., Naab, T., Walch, S., Burkert, A., and Heitsch, F. (2009b). Driving Turbulence and Triggering Star Formation by Ionizing Radiation. ApJL, 694:L26–L30.
Hansen, C. E., Klein, R. I., McKee, C. F., and Fisher, R. T. (2012). Feedback Effects on Low-mass Star Formation. ApJ, 747:22.
Harries, T. J. (2011). An algorithm for Monte Carlo time-dependent radiation transfer. MNRAS, 416:1500–1508.
Harries, T. J. (2015). Radiation-hydrodynamical simulations of massive star formation using Monte Carlo radiative transfer - I. Algorithms and numerical methods. MNRAS, 448:3156–3166.
Hartmann, L. and Kenyon, S. J. (1996). The FU Orionis Phenomenon. ARA&A, 34:207–240.
Haworth, T. J. and Harries, T. J. (2012). Radiation hydrodynamics of triggered star formation: the effect of the diffuse radiation field. MNRAS, 420:562–578.
Haworth, T. J., Harries, T. J., and Acreman, D. M. (2012). Testing diagnostics of triggered star formation. MNRAS, 426:203–217.
Haworth, T. J., Harries, T. J., Acreman, D. M., and Rundle, D. A. (2013). Assessing molecular line diagnostics of triggered star formation using synthetic observations. MNRAS, 431:3470–3484.
Hennebelle, P. and Iffrig, O. (2014). Simulations of magnetized multiphase galactic disc regulated by supernovae explosions. A&A, 570:A81.
Henney, W. J., Arthur, S. J., de Colle, F., and Mellema, G. (2009). Radiation-magnetohydrodynamic simulations of the photoionization of magnetized globules. MNRAS, 398:157–175.
Heyer, M., Krawczyk, C., Duval, J., and Jackson, J. M. (2009). Re-Examining Larson's Scaling Relationships in Galactic Molecular Clouds. ApJ, 699:1092–1103.
Hopkins, P. F. (2015). A new class of accurate, mesh-free hydrodynamic simulation methods. MNRAS, 450:53–110.
Hopkins, P. F., Cox, T. J., Hernquist, L., Narayanan, D., Hayward, C. C., and Murray, N. (2013). Star formation in galaxy mergers with realistic models of stellar feedback and the interstellar medium. MNRAS, 430:1901–1927.
Hopkins, P. F., Kereš, D., Oñorbe, J., Faucher-Giguère, C.-A., Quataert, E., Murray, N., and Bullock, J. S. (2014). Galaxies on FIRE (Feedback In Realistic Environments): stellar feedback explains cosmologically inefficient star formation. MNRAS, 445:581–603.
Hopkins, P. F., Quataert, E., and Murray, N. (2011). Self-regulated star formation in galaxies via momentum input from massive stars. MNRAS, 417:950–973.
Hopkins, P. F., Quataert, E., and Murray, N. (2012). The structure of the interstellar medium of star-forming galaxies. MNRAS, 421:3488–3521.
Hubber, D. A., Batty, C. P., McLeod, A., and Whitworth, A. P. (2011). SEREN - a new SPH code for star and planet formation simulations. Algorithms and tests. A&A, 529:A27.
Hubber, D. A., Walch, S., and Whitworth, A. P. (2013). An improved sink particle algorithm for SPH simulations. MNRAS, 430:3261–3275.
Iffrig, O. and Hennebelle, P. (2015). Mutual influence of supernovae and molecular clouds. A&A, 576:A95.
Johnson, J. L., Greif, T. H., and Bromm, V. (2007). Local Radiative Feedback in the Formation of the First Protogalaxies. ApJ, 665:85–95.
Katz, N. (1992). Dissipational galaxy formation. II - Effects of star formation. ApJ, 391:502–517.
Katz, N. and Gunn, J. E. (1991). Dissipational galaxy formation. I - Effects of gasdynamics. ApJ, 377:365–381.
Kawata, D., Gibson, B. K., Barnes, D. J., Grand, R. J. J., and Rahimi, A. (2014). Numerical simulations of bubble-induced star formation in dwarf irregular galaxies with a novel stellar feedback scheme. MNRAS, 438:1208–1222.
Kessel-Deynet, O. and Burkert, A. (2000). Ionizing radiation in smoothed particle hydrodynamics. MNRAS, 315:713–721.
Kim, C.-G., Kim, W.-T., and Ostriker, E. C. (2011). Regulation of Star Formation Rates in Multiphase Galactic Disks: Numerical Tests of the Thermal/Dynamical Equilibrium Model. ApJ, 743:25.
Kim, C.-G., Ostriker, E. C., and Kim, W.-T. (2013a). Three-dimensional Hydrodynamic Simulations of Multiphase Galactic Disks with Star Formation Feedback. I. Regulation of Star Formation Rates. ApJ, 776:1.
Kim, J.-h., Krumholz, M. R., Wise, J. H., Turk, M. J., Goldbaum, N. J., and Abel, T. (2013b). Dwarf Galaxies with Ionizing Radiation Feedback. I. Escape of Ionizing Photons. ApJ, 775:109.
Koo, B.-C. and McKee, C. F. (1992a). Dynamics of wind bubbles and superbubbles. I - Slow winds and fast winds. II - Analytic theory. ApJ, 388:93–126.
Koo, B.-C. and McKee, C. F. (1992b). Dynamics of Wind Bubbles and Superbubbles. II. Analytic Theory. ApJ, 388:103.
Koyama, H. and Inutsuka, S.-I. (2000). Molecular Cloud Formation in Shock-compressed Layers. ApJ, 532:980–993.
Koyama, H. and Ostriker, E. C. (2009). Gas Properties and Implications for Galactic Star Formation in Numerical Models of the Turbulent, Multiphase Interstellar Medium. ApJ, 693:1316–1345.
Krause, M., Fierlinger, K., Diehl, R., Burkert, A., Voss, R., and Ziegler, U. (2013). Feedback by massive stars and the emergence of superbubbles. I. Energy efficiency and Vishniac instabilities. A&A, 550:A49.
Kravtsov, A. V. (2003). On the Origin of the Global Schmidt Law of Star Formation. ApJL, 590:L1–L4.
Kravtsov, A. V., Klypin, A. A., and Khokhlov, A. M. (1997). Adaptive Refinement Tree: A New High-Resolution N-Body Code for Cosmological Simulations. ApJS, 111:73–94.
Krumholz, M. R., Bate, M. R., Arce, H. G., Dale, J. E., Gutermuth, R., Klein, R. I., Li, Z.-Y., Nakamura, F., and Zhang, Q. (2014). Star Cluster Formation and Feedback. Protostars and Planets VI, pages 243–266.
Krumholz, M. R., Cunningham, A. J., Klein, R. I., and McKee, C. F. (2010). Radiation Feedback, Fragmentation, and the Environmental Dependence of the Initial Mass Function. ApJ, 713:1120–1133.
Krumholz, M. R., Klein, R. I., and McKee, C. F. (2007a). Radiation-Hydrodynamic Simulations of Collapse and Fragmentation in Massive Protostellar Cores. ApJ, 656:959–979.
Krumholz, M. R., Klein, R. I., and McKee, C. F. (2011). Radiation-hydrodynamic Simulations of the Formation of Orion-like Star Clusters. I. Implications for the Origin of the Initial Mass Function. ApJ, 740:74.
Krumholz, M. R., Klein, R. I., and McKee, C. F. (2012). Radiation-hydrodynamic Simulations of the Formation of Orion-like Star Clusters. II. The Initial Mass Function from Winds, Turbulence, and Radiation. ApJ, 754:71.
Krumholz, M. R., Klein, R. I., McKee, C. F., Offner, S. S. R., and Cunningham, A. J. (2009). The Formation of Massive Star Systems by Accretion. Science, 323:754–.
Krumholz, M. R. and Matzner, C. D. (2009). The Dynamics of Radiation-pressure-dominated H II Regions. ApJ, 703:1352–1362.
Krumholz, M. R., Matzner, C. D., and McKee, C. F. (2006). The Global Evolution of Giant Molecular Clouds. I. Model Formulation and Quasi-Equilibrium Behavior. ApJ, 653:361–382.
Krumholz, M. R., Stone, J. M., and Gardiner, T. A. (2007b). Magnetohydrodynamic Evolution of H II Regions in Molecular Clouds: Simulation Methodology, Tests, and Uniform Media. ApJ, 671:518–535.
Krumholz, M. R. and Thompson, T. A. (2012). Direct Numerical Simulation of Radiation Pressure-driven Turbulence and Winds in Star Clusters and Galactic Disks. ApJ, 760:155.
Kuiper, R., Klahr, H., Beuther, H., and Henning, T. (2012a). A solution to the radiation pressure problem in the formation of massive stars. ArXiv e-prints.
Kuiper, R., Klahr, H., Beuther, H., and Henning, T. (2012b). On the stability of radiation-pressure-dominated cavities. A&A, 537:A122.
Kuiper, R., Klahr, H., Dullemond, C., Kley, W., and Henning, T. (2010). Fast and accurate frequency-dependent radiation transport for hydrodynamics simulations in massive star formation. A&A, 511:A81.
Lada, C. J., Lombardi, M., and Alves, J. F. (2010). On the Star Formation Rates in Molecular Clouds. ApJ, 724:687–693.
Lamers, H. J. G. L. M. and Cassinelli, J. P. (1999). Introduction to Stellar Winds.
Langer, N. (2012). Presupernova Evolution of Massive Single and Binary Stars. ARA&A, 50:107–164.
Leitherer, C., Robert, C., and Drissen, L. (1992). Deposition of mass, momentum, and energy by massive stars into the interstellar medium. ApJ, 401:596–617.
Leitherer, C., Schaerer, D., Goldader, J. D., Delgado, R. M. G., Robert, C., Kune, D. F., de Mello, D. F., Devost, D., and Heckman, T. M. (1999). Starburst99: Synthesis Models for Galaxies with Active Star Formation. ApJS, 123:3–40.
Li, Z.-Y. and Nakamura, F. (2006). Cluster Formation in Protostellar Outflow-driven Turbulence. ApJL, 640:L187–L190.
Mac Low, M.-M. and Klessen, R. S. (2004). Control of star formation by supersonic turbulence. Reviews of Modern Physics, 76:125–194.
Mac Low, M.-M., Smith, M. D., Klessen, R. S., and Burkert, A. (1998). The Decay of Supersonic and Super-Alfvénic Turbulence in Star-Forming Clouds. Ap&SS, 261:195–196.
Mackey, J., Gvaramadze, V. V., Mohamed, S., and Langer, N. (2015). Wind bubbles within H ii regions around slowly moving stars. A&A, 573:A10.
Mackey, J., Langer, N., and Gvaramadze, V. V. (2013). Dynamics of H II regions around exiled O stars. MNRAS, 436:859–880.
Mackey, J. and Lim, A. J. (2010). Dynamical models for the formation of elephant trunks in HII regions. MNRAS, 403:714–730.
Mackey, J. and Lim, A. J. (2011). Effects of magnetic fields on photoionized pillars and globules. MNRAS, 412:2079–2094.
Mackey, J., Mohamed, S., Gvaramadze, V. V., Kotak, R., Langer, N., Meyer, D. M.-A., Moriya, T. J., and Neilson, H. R. (2014). Interacting supernovae from photoionization-confined shells around red supergiant stars. Nature, 512:282–285.
MacLachlan, J. M., Bonnell, I. A., Wood, K., and Dale, J. E. (2015). Photoionising feedback and the star formation rates in galaxies. A&A, 573:A112.
Matzner, C. D. (2002). On the Role of Massive Stars in the Support and Destruction of Giant Molecular Clouds. ApJ, 566:302–314.
Matzner, C. D. (2007). Protostellar Outflow-driven Turbulence. ApJ, 659:1394–1403.
Matzner, C. D. and McKee, C. F. (1999). Bipolar Molecular Outflows Driven by Hydromagnetic Protostellar Winds. ApJL, 526:L109–L112.
McKee, C. F. and Tan, J. C. (2003). The Formation of Massive Stars from Turbulent Cores. ApJ, 585:850–871.
Medina, S.-N. X., Arthur, S. J., Henney, W. J., Mellema, G., and Gazol, A. (2014). Turbulence in simulated H II regions. MNRAS, 445:1797–1819.
Meidt, S. E., Schinnerer, E., García-Burillo, S., Hughes, A., Colombo, D., Pety, J., Dobbs, C. L., Schuster, K. F., Kramer, C., Leroy, A. K., Dumas, G., and Thompson, T. A. (2013). Gas Kinematics on Giant Molecular Cloud Scales in M51 with PAWS: Cloud Stabilization through Dynamical Pressure. ApJ, 779:45.
Mellema, G., Arthur, S. J., Henney, W. J., Iliev, I. T., and Shapiro, P. R. (2006a). Dynamical H II Region Evolution in Turbulent Molecular Clouds. ApJ, 647:397–403.
Mellema, G., Iliev, I. T., Alvarez, M. A., and Shapiro, P. R. (2006b). C 2-ray: A new method for photon-conserving transport of ionizing radiation. NewA, 11:374–395.
Moody, C. E., Guo, Y., Mandelker, N., Ceverino, D., Mozena, M., Koo, D. C., Dekel, A., and Primack, J. (2014). Star formation and clumps in cosmological galaxy simulations with radiation pressure feedback. MNRAS, 444:1389–1399.
Murray, N., Quataert, E., and Thompson, T. A. (2010). The Disruption of Giant Molecular Clouds by Radiation Pressure & the Efficiency of Star Formation in Galaxies. ApJ, 709:191–209.
Myers, A. T., Klein, R. I., Krumholz, M. R., and McKee, C. F. (2014). Star cluster formation in turbulent, magnetized dense clumps with radiative and outflow feedback. MNRAS, 439:3420–3438.
Nakamura, F. and Li, Z.-Y. (2007). Protostellar Turbulence Driven by Collimated Outflows. ApJ, 662:395–412.
Navarro, J. F. and White, S. D. M. (1994). Simulations of dissipative galaxy formation in hierarchically clustering universes-2. Dynamics of the baryonic component in galactic haloes. MNRAS, 267:401–412.
Nayakshin, S., Cha, S.-H., and Hobbs, A. (2009). Dynamic Monte Carlo radiation transfer in SPH: radiation pressure force implementation. MNRAS, 397:1314–1325.
Nenkova, M., Ivezić, Ž., and Elitzur, M. (2000). DUSTY: a Publicly Available Code for Modeling Dust Emission. Thermal Emission Spectroscopy and Analysis of Dust, Disks, and Regoliths, 196:77–82.
Ngoumou, J., Hubber, D., Dale, J. E., and Burkert, A. (2015). First Investigation of the Combined Impact of Ionizing Radiation and Momentum Winds from a Massive Star on a Self-gravitating Core. ApJ, 798:32.
Ntormousi, E., Burkert, A., Fierlinger, K., and Heitsch, F. (2011). Formation of Cold Filamentary Structure from Wind-blown Superbubbles. ApJ, 731:13.
Offner, S. S. R. and Arce, H. G. (2014). Investigations of Protostellar Outflow Launching and Gas Entrainment: Hydrodynamic Simulations and Molecular Emission. ApJ, 784:61.
Offner, S. S. R., Klein, R. I., McKee, C. F., and Krumholz, M. R. (2009). The Effects of Radiative Transfer on Low-Mass Star Formation. ApJ, 703:131–149.
Okamoto, T., Eke, V. R., Frenk, C. S., and Jenkins, A. (2005). Effects of feedback on the morphology of galaxy discs. MNRAS, 363:1299–1314.
Osterbrock, D. E. and Ferland, G. J. (2006). Astrophysics of gaseous nebulae and active galactic nuclei.
Ostriker, E. C. and Shetty, R. (2011). Maximally Star-forming Galactic Disks. I. Starburst Regulation Via Feedback-driven Turbulence. ApJ, 731:41.
Ostriker, J. P. and McKee, C. F. (1988). Astrophysical blastwaves. Reviews of Modern Physics, 60:1–68.
Pawlik, A. H., Milosavljević, M., and Bromm, V. (2013). The First Galaxies: Assembly under Radiative Feedback from the First Stars. ApJ, 767:59.
Pawlik, A. H. and Schaye, J. (2008). TRAPHIC - radiative transfer for smoothed particle hydrodynamics simulations. MNRAS, 389:651–677.
Pawlik, A. H., Schaye, J., and Dalla Vecchia, C. (2015). Spatially adaptive radiation-hydrodynamical simulations of galaxy formation during cosmological reionization. ArXiv e-prints.
Pelupessy, F. I. and Portegies Zwart, S. (2012). The evolution of embedded star clusters. MNRAS, 420:1503–1517.
Peters, T., Banerjee, R., Klessen, R. S., and Mac Low, M.-M. (2011). The Interplay of Magnetic Fields, Fragmentation, and Ionization Feedback in High-mass Star Formation. ApJ, 729:72.
Peters, T., Banerjee, R., Klessen, R. S., Mac Low, M.-M., Galván-Madrid, R., and Keto, E. R. (2010). H II Regions: Witnesses to Massive Star Formation. ApJ, 711:1017–1028.
Peters, T., Klaassen, P. D., Mac Low, M.-M., Schrön, M., Federrath, C., Smith, M. D., and Klessen, R. S. (2014). Collective Outflow from a Small Multiple Stellar System. ApJ, 788:14.
Petkova, M. and Springel, V. (2009). An implementation of radiative transfer in the cosmological simulation code GADGET. MNRAS, 396:1383–1403.
Petkova, M. and Springel, V. (2011). Simulations of galaxy formation with radiative transfer: hydrogen reionization and radiative feedback. MNRAS, 412:935–946.
Plewa, T. (1995). Fast radiative shocks in dense media - III. Properties of the emission. MNRAS, 275:143–152.
Price, D. J. and Bate, M. R. (2009). Inefficient star formation: the combined effects of magnetic fields and radiative feedback. MNRAS, 398:33–46.
Read, J. I., Hayfield, T., and Agertz, O. (2010). Resolving mixing in smoothed particle hydrodynamics. MNRAS, 405:1513–1530.
Renaud, F., Bournaud, F., Emsellem, E., Elmegreen, B., Teyssier, R., Alves, J., Chapon, D., Combes, F., Dekel, A., Gabor, J., Hennebelle, P., and Kraljic, K. (2013). A sub-parsec resolution simulation of the Milky Way: global structure of the interstellar medium and properties of molecular clouds. MNRAS, 436:1836–1851.
Rijkhorst, E.-J., Plewa, T., Dubey, A., and Mellema, G. (2006). Hybrid characteristics: 3D radiative transfer for parallel adaptive mesh refinement hydrodynamics. A&A, 452:907–920.
Robertson, B., Yoshida, N., Springel, V., and Hernquist, L. (2004). Disk Galaxy Formation in a Λ Cold Dark Matter Universe. ApJ, 606:32–45.
Rogers, H. and Pittard, J. M. (2013). Feedback from winds and supernovae in massive stellar clusters - I. Hydrodynamics. MNRAS, 431:1337–1351.
Rosen, A. L., Lopez, L. A., Krumholz, M. R., and Ramirez-Ruiz, E. (2014). Gone with the wind: Where is the missing stellar wind energy from massive star clusters? MNRAS, 442:2701–2716.
Roškar, R., Teyssier, R., Agertz, O., Wetzstein, M., and Moore, B. (2014). A systematic look at the effects of radiative feedback on disc galaxy formation. MNRAS, 444:2837–2853.
Saitoh, T. R. and Makino, J. (2013). A Density-independent Formulation of Smoothed Particle Hydrodynamics. ApJ, 768:44.
Sales, L. V., Marinacci, F., Springel, V., and Petkova, M. (2014). Stellar feedback by radiation pressure and photoionization. MNRAS, 439:2990–3006.
Sandford, II, M. T., Whitaker, R. W., and Klein, R. I. (1982). Radiation-driven implosions in molecular clouds. ApJ, 260:183–201.
Sawala, T., Scannapieco, C., Maio, U., and White, S. (2010). Formation of isolated dwarf galaxies with feedback. MNRAS, 402:1599–1613.
Scannapieco, C., Tissera, P. B., White, S. D. M., and Springel, V. (2006). Feedback and metal enrichment in cosmological SPH simulations - II. A multiphase model with supernova energy feedback. MNRAS, 371:1125–1139.
Scannapieco, C., Tissera, P. B., White, S. D. M., and Springel, V. (2008). Effects of supernova feedback on the formation of galaxy discs. MNRAS, 389:1137–1149.
Scannapieco, C., Wadepuhl, M., Parry, O. H., Navarro, J. F., Jenkins, A., Springel, V., Teyssier, R., Carlson, E., Couchman, H. M. P., Crain, R. A., Dalla Vecchia, C., Frenk, C. S., Kobayashi, C., Monaco, P., Murante, G., Okamoto, T., Quinn, T., Schaye, J., Stinson, G. S., Theuns, T., Wadsley, J., White, S. D. M., and Woods, R. (2012). The Aquila comparison project: the effects of feedback and numerical methods on simulations of galaxy formation. MNRAS, 423:1726–1749.
Schaye, J. (2004). Star Formation Thresholds and Galaxy Edges: Why and Where. ApJ, 609:667–682.
Schaye, J., Crain, R. A., Bower, R. G., Furlong, M., Schaller, M., Theuns, T., Dalla Vecchia, C., Frenk, C. S., McCarthy, I. G., Helly, J. C., Jenkins, A., Rosas-Guevara, Y. M., White, S. D. M., Baes, M., Booth, C. M., Camps, P., Navarro, J. F., Qu, Y., Rahmati, A., Sawala, T., Thomas, P. A., and Trayford, J. (2015). The EAGLE project: simulating the evolution and assembly of galaxies and their environments. MNRAS, 446:521–554.
Schaye, J. and Dalla Vecchia, C. (2008). On the relation between the Schmidt and Kennicutt-Schmidt star formation laws and its implications for numerical simulations. MNRAS, 383:1210–1222.
Shetty, R. and Ostriker, E. C. (2008). Cloud and Star Formation in Disk Galaxy Models with Feedback. ApJ, 684:978–995.
Shetty, R. and Ostriker, E. C. (2012). Maximally Star-forming Galactic Disks. II. Vertically Resolved Hydrodynamic Simulations of Starburst Regulation. ApJ, 754:2.
Silich, S. and Tenorio-Tagle, G. (2013). How Significant is Radiation Pressure in the Dynamics of the Gas around Young Stellar Clusters? ApJ, 765:43.
Simpson, C. M., Bryan, G. L., Johnston, K. V., Smith, B. D., Mac Low, M.-M., Sharma, S., and Tumlinson, J. (2013). The effect of feedback and reionization on star formation in low-mass dwarf galaxy haloes. MNRAS, 432:1989–2011.
Slyz, A. D., Devriendt, J. E. G., Bryan, G., and Silk, J. (2005). Towards simulating star formation in the interstellar medium. MNRAS, 356:737–752.
Smith, N. (2006). A census of the Carina Nebula - I. Cumulative energy input from massive stars. MNRAS, 367:763–772.
Smith, R. J., Glover, S. C. O., Clark, P. C., Greif, T., and Klessen, R. S. (2011). The effects of accretion luminosity upon fragmentation in the early universe. MNRAS, 414:3633–3644.
Smith, R. J., Glover, S. C. O., Clark, P. C., Klessen, R. S., and Springel, V. (2014). CO-dark gas and molecular filaments in Milky Way-type galaxies. MNRAS, 441:1628–1645.
Spitzer, L. (1978). Physical processes in the interstellar medium.
Springel, V. (2010a). E pur si muove: Galilean-invariant cosmological hydrodynamical simulations on a moving mesh. MNRAS, 401:791–851.
Springel, V. (2010b). Smoothed Particle Hydrodynamics in Astrophysics. ARA&A, 48:391–430.
Springel, V. and Hernquist, L. (2003). Cosmological smoothed particle hydrodynamics simulations: a hybrid multiphase model for star formation. MNRAS, 339:289–311.
Stamatellos, D., Whitworth, A. P., Bisbas, T., and Goodwin, S. (2007). Radiative transfer and the energy equation in SPH simulations of star formation. A&A, 475:37–49.
Stamatellos, D., Whitworth, A. P., and Hubber, D. A. (2011). The Importance of Episodic Accretion for Low-mass Star Formation. ApJ, 730:32.
Stamatellos, D., Whitworth, A. P., and Hubber, D. A. (2012). Episodic accretion, protostellar radiative feedback, and their role in low-mass star formation. MNRAS, 427:1182–1193.
Stinson, G. S., Brook, C., Macciò, A. V., Wadsley, J., Quinn, T. R., and Couchman, H. M. P. (2013). Making Galaxies In a Cosmological Context: the need for early stellar feedback. MNRAS, 428:129–140.
Stinson, G. S., Dalcanton, J. J., Quinn, T., Kaufmann, T., and Wadsley, J. (2007). Breathing in Low-Mass Galaxies: A Study of Episodic Star Formation. ApJ, 667:170–175.
Strömgren, B. (1939). The Physical State of Interstellar Hydrogen. ApJ, 89:526.
Sugitani, K., Fukui, Y., and Ogura, K. (1991). A catalog of bright-rimmed clouds with IRAS point sources: Candidates for star formation by radiation-driven implosion. I - The Northern Hemisphere. ApJS, 77:59–66.
Tasker, E. J. and Bryan, G. L. (2006). Simulating Star Formation and Feedback in Galactic Disk Models. ApJ, 641:878–890.
Tasker, E. J. and Tan, J. C. (2009). Star Formation in Disk Galaxies. I. Formation and Evolution of Giant Molecular Clouds via Gravitational Instability and Cloud Collisions. ApJ, 700:358–375.
Tenorio-Tagle, G. (1979). The gas dynamics of H II regions. I - The champagne model. A&A, 71:59–65.
Tenorio-Tagle, G., Bodenheimer, P., and Yorke, H. W. (1985). Non-spherical supernova remnants. II - The interaction of remnants with molecular clouds. A&A, 145:70–80.
Teyssier, R., Pontzen, A., Dubois, Y., and Read, J. I. (2013). Cusp-core transformations in dwarf galaxies: observational predictions. MNRAS, 429:3068–3078.
Toalá, J. A. and Arthur, S. J. (2011). Radiation-hydrodynamic Models of the Evolving Circumstellar Medium around Massive Stars. ApJ, 737:100.
Trac, H. Y. and Gnedin, N. Y. (2011). Computer Simulations of Cosmic Reionization. Advanced Science Letters, 4:228–243.
Tremblin, P., Audit, E., Minier, V., Schmidt, W., and Schneider, N. (2012a). Three-dimensional simulations of globule and pillar formation around HII regions: turbulence and shock curvature. A&A, 546:A33.
Tremblin, P., Audit, E., Minier, V., and Schneider, N. (2012b). 3D simulations of pillar formation around HII regions: the importance of shock curvature. A&A, 538:A31.
Tremblin, P., Minier, V., Schneider, N., Audit, E., Hill, T., Didelon, P., Peretto, N., Arzoumanian, D., Motte, F., Zavagno, A., Bontemps, S., Anderson, L. D., André, P., Bernard, J. P., Csengeri, T., Di Francesco, J., Elia, D., Hennemann, M., Könyves, V., Marston, A. P., Nguyen Luong, Q., Rivera-Ingraham, A., Roussel, H., Sousbie, T., Spinoglio, L., White, G. J., and Williams, J. (2013). Pillars and globules at the edges of H ii regions. Confronting Herschel observations and numerical simulations. A&A, 560:A19.
Turner, N. J. and Stone, J. M. (2001). A Module for Radiation Hydrodynamic Calculations with ZEUS-2D Using Flux-limited Diffusion. ApJS, 135:95–107.
Übler, H., Naab, T., Oser, L., Aumer, M., Sales, L. V., and White, S. D. M. (2014). Why stellar feedback promotes disc formation in simulated galaxies. MNRAS, 443:2092–2111.
Urban, A., Evans, II, N. J., and Doty, S. D. (2009). A Parameter Study of the Dust and Gas Temperature in a Field of Young Stars. ApJ, 698:1341–1356.
Valdivia, V. and Hennebelle, P. (2014). A fast tree-based method for estimating column densities in adaptive mesh refinement codes. Influence of UV radiation field on the structure of molecular clouds. A&A, 571:A46.
Vázquez-Semadeni, E., Colín, P., Gómez, G. C., Ballesteros-Paredes, J., and Watson, A. W. (2010). Molecular Cloud Evolution. III. Accretion Versus Stellar Feedback. ApJ, 715:1302–1317.
Wada, K. and Norman, C. A. (2001). Numerical Models of the Multiphase Interstellar Matter with Stellar Energy Feedback on a Galactic Scale. ApJ, 547:172–186.
Wada, K. and Norman, C. A. (2007). Density Structure of the Interstellar Medium and the Star Formation Rate in Galactic Disks. ApJ, 660:276–287.
Walch, S., Whitworth, A. P., Bisbas, T. G., Wünsch, R., and Hubber, D. A. (2013). Clumps and triggered star formation in ionized molecular clouds. MNRAS, 435:917–927.
Walch, S. K., Girichidis, P., Naab, T., Gatto, A., Glover, S. C. O., Wünsch, R., Klessen, R. S., Clark, P. C., Peters, T., and Baczynski, C. (2014). The SILCC (SImulating the LifeCycle of molecular Clouds) project: I. Chemical evolution of the supernova-driven ISM. ArXiv e-prints.
Walch, S. K. and Naab, T. (2014). The energy and momentum input of supernova explosions in structured and ionised molecular clouds. ArXiv e-prints.
Walch, S. K., Whitworth, A. P., Bisbas, T., Wünsch, R., and Hubber, D. (2012). Dispersal of molecular clouds by ionizing radiation. MNRAS, 427:625–636.
Wang, P., Li, Z.-Y., Abel, T., and Nakamura, F. (2010). Outflow Feedback Regulated Massive Star Formation in Parsec-Scale Cluster-Forming Clumps. ApJ, 709:27–41.
Weaver, R., McCray, R., Castor, J., Shapiro, P., and Moore, R. (1977). Interstellar bubbles. II - Structure and evolution. ApJ, 218:377–395.
Weidner, C. and Vink, J. S. (2010). The masses, and the mass discrepancy of O-type stars. A&A, 524:A98.
Whalen, D. and Norman, M. L. (2006). A Multistep Algorithm for the Radiation Hydrodynamical Transport of Cosmological Ionization Fronts and Ionized Flows. ApJS, 162:281–303.
Whalen, D. and Norman, M. L. (2008). Ionization Front Instabilities in Primordial H II Regions. ApJ, 673:664–675.
Whalen, D., O'Shea, B. W., Smidt, J., and Norman, M. L. (2008). How the First Stars Regulated Local Star Formation. I. Radiative Feedback. ApJ, 679:925–941.
Whitehouse, S. C., Bate, M. R., and Monaghan, J. J. (2005). A faster algorithm for smoothed particle hydrodynamics with radiative transfer in the flux-limited diffusion approximation. MNRAS, 364:1367–1377.
Whitmore, B. C., Chandar, R., Schweizer, F., Rothberg, B., Leitherer, C., Rieke, M., Rieke, G., Blair, W. P., Mengel, S., and Alonso-Herrero, A. (2010). The Antennae Galaxies (NGC 4038/4039) Revisited: Advanced Camera for Surveys and NICMOS Observations of a Prototypical Merger. AJ, 140:75–109.
Whitworth, A. P., Bhattal, A. S., Chapman, S. J., Disney, M. J., and Turner, J. A. (1994). Fragmentation of shocked interstellar gas layers. A&A, 290:421–427.
Wise, J. H. and Abel, T. (2011). ENZO+MORAY: radiation hydrodynamics adaptive mesh refinement simulations with adaptive ray tracing. MNRAS, 414:3458–3491.
Wise, J. H., Abel, T., Turk, M. J., Norman, M. L., and Smith, B. D. (2012). The birth of a galaxy - II. The role of radiation pressure. MNRAS, 427:311–326.
Wood, D. O. S. and Churchwell, E. (1989). The morphologies and physical properties of ultracompact H II regions. ApJS, 69:831–895.
Wood, K., Mathis, J. S., and Ercolano, B. (2004). A three-dimensional Monte Carlo photoionization code for modelling diffuse ionized gas. MNRAS, 348:1337–1347.
Wünsch, R., Tenorio-Tagle, G., Palouš, J., and Silich, S. (2008). Two-dimensional Hydrodynamic Models of Super Star Clusters with a Positive Star Formation Feedback. ApJ, 683:683–692.
Yorke, H. W., Tenorio-Tagle, G., Bodenheimer, P., and Rozyczka, M. (1989). The combined role of ionization and supernova explosions in the destruction of molecular clouds. A&A, 216:207–214.