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- W20984979 abstract "We present a further analysis of the CO(1-0) and CO(2-1) survey of nearby galaxies carried out at the IRAM 30 meter telescope. Along with existing data for total gas masses, our data indicate that there is more CO emission in tidally perturbed galaxies, and that this emission is more centrally concentrated. This could be interpreted as being due to a different N H2 /W CO conversion ratio. However, since the excitation (as measured by the line ratio) of the gas is not highly different in isolated and perturbed galaxies (Papers I and II), we will assume that the standard N H2 /W CO conversion ratio is valid for all galaxies (except for NGC 3310, where the line ratio is ≥2). In this case, our data suggest that there is more molecular gas in disturbed galaxies" @default.
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- W20984979 date "1993-03-01" @default.
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- W20984979 title "A CO (1-0) and CO (2-1) survey of nearby spiral galaxies. III. More H2 gas in perturbed galaxies ?" @default.
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