A new empirical method to estimate the molecular gas mass in galaxies. (2nd May 2019)

• Record Type: Journal Article
• Authors: Concas, Alice; Popesso, Paola
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 486:Number 1(2019)
• Page Start: L91
• Page End: L95
• Publication Date: 2019-05-02
• Subjects: galaxies: ISM -- ISM: molecules -- (ISM:) dust, extinction; Astronomy -- Research -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnrasl/slz065
• Languages: English
• ISSNs: 1745-3933

Abstract

ABSTRACT: We find a tight correlation between the dust extinction, traced by the Balmer Decrement (BD = H α/H β), the CO(1-0) line luminosity ( L CO ), and total molecular gas mass ( M H2 ) in a sample of 222 local star-forming galaxies drawn from the xCOLD GASS survey. As expected, the galaxy disc inclination affects the correlation by inducing a saturation of the Balmer decrement on highly inclined galaxies. Once this effect is taken into account, L CO and M H2 can be expressed as a function of BD with a scatter of ∼0.3 dex. We do not find any dependence on galaxy size, mass, morphology, star formation activity, and gas metallicity. The correlation disappears if the atomic gas phase is considered. This is likely due to the fact that the region traced by the BD, the stellar disc, is much smaller than the HI disc.