NASA/IPAC EXTRAGALACTIC DATABASE
Date and Time of the Query: 2019-06-19 T23:16:00 PDT
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For refcode 1999A&A...343...51A:
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Copyright by European Southern Observatory (ESO). Reproduced by permission
1999A&A...343...51A Dust outflows from starburst galaxies. ALTON P.B., DAVIES J.I., BIANCHI S. Received 11 September 1998/Accepted 2 December 1998 Abstract: We present submillimeter SCUBA images of the nearby, starburst galaxies NGC 253, NGC 4631 and M82 (primarily at wavelengths of 450 and 850 microns). The edge-on orientation of our targets, in conjunction with the resolution of the instrument (15" FWHM at 850 microns), allows us to probe the optically-obscured centre and resolve the minor-axis superwind from the main disk. For NGC 253 and M82, we detect a bright source, a few hundred parsec in diameter, which corresponds to the central starburst. In the case of M82, the bi-lobal nature of the central source is suggestive of a torus or ring. We confirm the existence of a dust outflow along the minor axis of M82 and make a similar (but somewhat more tentative report) for the other two galaxies NGC 253 and NGC 4631. The scale-size of the `vertical' features is 0.7-1.2kpc. A mass of 10^6-7^M_sun_ is inferred for the outflowing grains in M82. We conclude that this amount of grain material could either have accrued from an inflow along the disk (e.g. a bar) or, if the lower mass limit applies, have been synthesized by massive stars in the starburst. The ejected grains are probably traveling close to the escape velocity of the host galaxy and assuming, hypothetically, that they do manage to breach the halo, we expect superwinds to expel up to 10% of the dust residing in interstellar disks into the intergalactic medium. Key words: ISM: dust, extinction - galaxies: active - galaxies: intergalactic medium - galaxies: jets - galaxies: starburst - infrared: galaxies
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