Astronomy and Astrophysics – Astrophysics
Scientific paper
2006-09-25
Astron.Rep. 50 (2006) 626-637
Astronomy and Astrophysics
Astrophysics
11 pages,7 figures, published in Astronomy Reports
Scientific paper
10.1134/S1063772906080038
A sample of 66 galaxies from the catalog of Bettoni et al. (CISM) with anomalously high molecular-to-atomic hydrogen mass ratios (M_{mol}/M_{HI}>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 $H_2$ is due to transition of HI to H_2. Galaxies with bars and active nuclei are found more frequently among galaxies which have M_{mol} estimates in CISM. In a small fraction of galaxies, high M_{mol}/M_{HI} ratios are caused by the overestimation of M_{mol} due to a low conversion factor for the translation of CO-line intensities into the number of H_2 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 M_{mol}/M_{HI} ratios.
Kasparova A. V.
Zasov Anatoli V.
No associations
LandOfFree
Galaxies with unusually high abundances of molecular hydrogen does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Galaxies with unusually high abundances of molecular hydrogen, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Galaxies with unusually high abundances of molecular hydrogen will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-14770