The distribution of neutral hydrogen in the colour–magnitude plane of galaxies
Abstract
ABSTRACT We present the conditional H i (neutral hydrogen) mass function (HIMF) conditioned on observed optical properties, Mr (r-band absolute magnitude), and Cur (u − r colour), for a sample of 7709 galaxies from Arecibo Legacy Fast ALFA (40 per cent data release – α.40) which overlaps with a common volume in SDSS DR7. Based on the conditional HIMF, we find that the luminous red, luminous blue, and faint blue populations dominate the total HIMF at the high-mass end, knee, and the low-mass end, respectively. We use the conditional HIMF to derive the underlying distribution function of ΩH i (H i density parameter), p(ΩH i), in the colour–magnitude plane of galaxies. The distribution, p(ΩH i), peaks in the blue cloud at $$\mathit{ M_{{r}}}^{\text{max}}=-19.25, \mathit{ C_{{ur}}}^{\text{max}}=1.44$$ but is skewed. It has a long tail towards faint blue galaxies, and luminous red galaxies. We argue that p(ΩH i) can be used to reveal the underlying relation between cold gas, stellar mass, and the star formation rate in an unbiased way, that is, the derived relation does not suffer from survey or sample selection.
- Authors:
- Publication Date:
- Sponsoring Org.:
- USDOE
- OSTI Identifier:
- 1774690
- Resource Type:
- Published Article
- Journal Name:
- Monthly Notices of the Royal Astronomical Society: Letters
- Additional Journal Information:
- Journal Name: Monthly Notices of the Royal Astronomical Society: Letters Journal Volume: 500 Journal Issue: 1; Journal ID: ISSN 1745-3925
- Publisher:
- Oxford University Press
- Country of Publication:
- United Kingdom
- Language:
- English
Citation Formats
Dutta, Saili, and Khandai, Nishikanta. The distribution of neutral hydrogen in the colour–magnitude plane of galaxies. United Kingdom: N. p., 2020.
Web. doi:10.1093/mnrasl/slaa178.
Dutta, Saili, & Khandai, Nishikanta. The distribution of neutral hydrogen in the colour–magnitude plane of galaxies. United Kingdom. https://doi.org/10.1093/mnrasl/slaa178
Dutta, Saili, and Khandai, Nishikanta. Sat .
"The distribution of neutral hydrogen in the colour–magnitude plane of galaxies". United Kingdom. https://doi.org/10.1093/mnrasl/slaa178.
@article{osti_1774690,
title = {The distribution of neutral hydrogen in the colour–magnitude plane of galaxies},
author = {Dutta, Saili and Khandai, Nishikanta},
abstractNote = {ABSTRACT We present the conditional H i (neutral hydrogen) mass function (HIMF) conditioned on observed optical properties, Mr (r-band absolute magnitude), and Cur (u − r colour), for a sample of 7709 galaxies from Arecibo Legacy Fast ALFA (40 per cent data release – α.40) which overlaps with a common volume in SDSS DR7. Based on the conditional HIMF, we find that the luminous red, luminous blue, and faint blue populations dominate the total HIMF at the high-mass end, knee, and the low-mass end, respectively. We use the conditional HIMF to derive the underlying distribution function of ΩH i (H i density parameter), p(ΩH i), in the colour–magnitude plane of galaxies. The distribution, p(ΩH i), peaks in the blue cloud at $\mathit{ M_{{r}}}^{\text{max}}=-19.25, \mathit{ C_{{ur}}}^{\text{max}}=1.44$ but is skewed. It has a long tail towards faint blue galaxies, and luminous red galaxies. We argue that p(ΩH i) can be used to reveal the underlying relation between cold gas, stellar mass, and the star formation rate in an unbiased way, that is, the derived relation does not suffer from survey or sample selection.},
doi = {10.1093/mnrasl/slaa178},
journal = {Monthly Notices of the Royal Astronomical Society: Letters},
number = 1,
volume = 500,
place = {United Kingdom},
year = {Sat Oct 31 00:00:00 EDT 2020},
month = {Sat Oct 31 00:00:00 EDT 2020}
}
https://doi.org/10.1093/mnrasl/slaa178
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