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19972023
most citedxCOLD GASS: the complete IRAM-30m legacy survey of molecular gas for galaxy evolution studies

526 citations · 5.9k across the 76 of their papers we have counts for

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Showing 2019Show all

8 papers · 1 filter

astro-ph.GA2019★ 9 cited

The growth of bulges and discs in relatively HI-rich galaxies: indication from HI scaling relations

Xinkai Chen, Jing Wang, Xu Kong +3

We study the relation between the properties of the bulge/disc components and the HI mass fraction of galaxies. We find that at fixed stellar mass, disc colours are correlated with…

astro-ph.GA2019★ 6 cited

The evolution of baryonic mass function of galaxies to z=3

Zhizheng Pan, Yingjie Peng, Xianzhong Zheng +2

We combine the published stellar mass function (SMF) and gas scaling relations to explore the baryonic (stellar plus cold gas) mass function (BMF) of galaxies to redshift . We…

astro-ph.GA2019★ 48 cited

Origin of the galaxy HI size-mass relation

Adam R. H. Stevens, Benedikt Diemer, Claudia del P. Lagos +4

We analytically derive the observed size-mass relation of galaxies' atomic hydrogen (HI), including limits on its scatter, based on simple assumptions about the structure of HI dis…

astro-ph.GA2019★ 114 cited

Further evidence for a population of dark-matter-deficient dwarf galaxies

Qi Guo, Huijie Hu, Zheng Zheng +9

In the standard cosmological model, dark matter drives the structure formation and constructs potential wells within which galaxies may form. The baryon fraction in dark halos can…

astro-ph.GA2019★ 17 cited

Complex distribution and velocity field of molecular gas in NGC 1316 as revealed by Morita Array of ALMA

Kana Morokuma-Matsui, Paolo Serra, Filippo M. Maccagni +11

We present the results of CO(=1-0) mosaicing observations of the cD galaxy NGC 1316 at kpc-resolution performed with the Morita Array of the Atacama Large Millimeter/subm…

astro-ph.GA2019★ 110 cited

The Local Volume HI Survey (LVHIS)

Bärbel S. Koribalski, Jing Wang, Peter Kamphuis +8

The `Local Volume HI Survey' (LVHIS) comprises deep HI spectral line and 20-cm radio continuum observations of 82 nearby, gas-rich galaxies, supplemented by multi-wavelength images…