Galaxies with unusually high abundances of molecular hydrogen
Abstract
A sample of 66 galaxies from the catalog of Bettoni et al. (CISM) with anomalously high molecular-to-atomic hydrogen mass ratios (Mmol/MHI>2) is considered. The sample galaxies do not differ systematically from other galaxies in the catalog with the same morphological types, in terms of their photometric parameters, rotational velocities, dust contents, or the total mass of gas in comparison with galaxies of similar linear sizes and disk angular momentum. This suggests that the overabundance of H2 is due to transition of HI to H2. Galaxies with bars and active nuclei are found more frequently among galaxies which have Mmol estimates in CISM. In a small fraction of galaxies, high Mmol/MHI ratios are caused by the overestimation of Mmol due to a low conversion factor for the translation of CO-line intensities into the number of H2 molecules along the line of sight. It is argued that the "molecularization" of the bulk of the gas mass could be due 1) to the concentration of gas in the inner regions of the galactic disks, resulting to a high gas pressure and 2) to relatively low star-formation rate per unit mass of molecular gas which indeed takes place in galaxies with high Mmol/MHI ratios.
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