2012ApJ...751..127M -
Astrophys. J., 751, 127 (2012/June-1)
Observational constraints on the molecular gas content in nearby starburst dwarf galaxies.
McQUINN K.B.W., SKILLMAN E.D., DALCANTON J.J., DOLPHIN A.E., CANNON J.M., HOLTZMAN J., WEISZ D.R. and WILLIAMS B.F.
Abstract (from CDS):
Using star formation histories derived from optically resolved stellar populations in 19 nearby starburst dwarf galaxies observed with the Hubble Space Telescope, we measure the stellar mass surface densities of stars newly formed in the bursts. By assuming a star formation efficiency (SFE), we then calculate the inferred gas surface densities present at the onset of the starbursts. Assuming an SFE of 1%, as is often assumed in normal star-forming galaxies, and assuming that the gas was purely atomic, translates to very high H I surface densities (∼102-103 M☉/pc2), which are much higher than have been observed in dwarf galaxies. This implies either higher values of SFE in these dwarf starburst galaxies or the presence of significant amounts of H2 in dwarfs (or both). Raising the assumed SFEs to 10% or greater (in line with observations of more massive starbursts associated with merging galaxies), still results in H I surface densities higher than observed in 10 galaxies. Thus, these observations appear to require that a significant fraction of the gas in these dwarf starbursts galaxies was in the molecular form at the onset of the bursts. Our results imply molecular gas column densities in the range 1019-1021/cm2 for the sample. In the galaxies where CO observations have been made, these densities correspond to values of the CO-H2 conversion factor (XCO) in the range >(3-80) x1020/cm2 (K km/s)–1, or up to 40xgreater than Galactic XCO values.
Abstract Copyright:
∼
Journal keyword(s):
galaxies: dwarf - galaxies: evolution - galaxies: starburst
Simbad objects:
22
Full paper
View the references in ADS
To bookmark this query, right click on this link: simbad:2012ApJ...751..127M and select 'bookmark this link' or equivalent in the popup menu