NASA/IPAC EXTRAGALACTIC DATABASE
Date and Time of the Query: 2019-05-24 T19:13:11 PDT
Help | Comment | NED Home

For refcode 2018A&A...609A.102R:
Retrieve 8 NED objects in this reference.
Please click here for ADS abstract

NED Abstract

Copyright by European Southern Observatory (ESO). Reproduced by permission
2018A&A...609A.102R Inner and outer star forming regions over the disks of spiral galaxies. I. Sample characterization Rodriguez-Baras, M.; Diaz, A. I.; Rosales-Ortega, F. F.; Sanchez, S. F. Abstract. Context. The knowledge of abundance distributions is central to understanding the formation and evolution of galaxies. Most of the relations employed for the derivation of gas abundances have so far been derived from observations of outer disk H II regions, despite the known differences between inner and outer regions. Aims: Using integral field spectroscopy (IFS) observations we aim to perform a systematic study and comparison of two inner and outer H II regions samples. The spatial resolution of the IFS, the number of objects and the homogeneity and coherence of the observations allow a complete characterization of the main observational properties and differences of the regions. Methods: We analyzed a sample of 725 inner H II regions and a sample of 671 outer H II regions, all of them detected and extracted from the observations of a sample of 263 nearby, isolated, spiral galaxies observed by the CALIFA survey. Results: We find that inner H II regions show smaller equivalent widths, greater extinction and luminosities, along with greater values of [N II] lambda6583/Halpha and [O II] lambda3727/[O III] lambda5007 emission-line ratios, indicating higher metallicities and lower ionization parameters. Inner regions have also redder colors and higher photometric and ionizing masses, although M_ion_M_phot_ is slighty higher for the outer regions. Conclusions: This work shows important observational differences between inner and outer H II regions in star forming galaxies not previously studied in detail. These differences indicate that inner regions have more evolved stellar populations and are in a later evolution state with respect to outer regions, which goes in line with the inside-out galaxy formation paradigm. Table 4 is only available at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/609/A102 Key words: methods: data analysis, techniques: imaging spectroscopy, galaxies: spiral, Hii regions
Retrieve 8 NED objects in this reference.
Please click here for ADS abstract

Back to NED Home