The dark matter haloes of HI selected galaxies

Dutta, Saili; Khandai, Nishikanta; Rana, Sandeep

doi:10.1093/mnras/stab3618

The dark matter haloes of HI selected galaxies

Journal Article · Sat Dec 11 00:00:00 EST 2021 · Monthly Notices of the Royal Astronomical Society

DOI:https://doi.org/10.1093/mnras/stab3618· OSTI ID:1982570

^[1]; ^[1]; Rana, Sandeep ^[1]

National Institute of Science Education and Research (NISER), Jatni (India)

We present the neutral hydrogen mass (M_HI) function (HIMF) and velocity width (w₅₀) function (HIWF) based on a sample of 7857 galaxies from the 40 per cent data release of the ALFALFA survey (α.40). The low mass (velocity width) end of the HIMF (HIWF) is dominated by the blue population of galaxies whereas the red population dominates the HIMF (HIWF) at the high mass (velocity width) end. We use a deconvolution method to estimate the HI rotational velocity (V_rot) functions (HIVF) from the HIWF for the total, red, and blue samples. The HIWF and HIVF for the red and blue samples are well separated at the knee of the function compared to their HIMFs. We then use recent stacking results from the ALFALFA survey to constrain the halo mass (M_h) function of HI-selected galaxies. This allows us to obtain various scaling relations between M_HI–w₅₀–V_rot–M_h, which we present. The M_HI–M_h relation has a steep slope ~2.10 at small masses and flattens to ~0.34 at masses larger than a transition halo mass, $$\log _{10}(M_{\rm{ht}}h_{70}^2/M_{\odot })=10.62$$. Our scaling relation is robust and consistent with a volume-limited sample of α.40. The M_HI–M_h relation is qualitatively similar to the M_star–M_h relation but the transition halo mass is smaller by ~1.4 dex compared to that of the M_star–M_h relation. Our results suggest that baryonic processes like heating and feedback in larger mass haloes suppress HI gas on a shorter time-scale compared to star formation.

View Accepted Manuscript (DOE)

Research Organization:: US Department of Energy (USDOE), Washington, DC (United States). Office of Science, Sloan Digital Sky Survey (SDSS)

Sponsoring Organization:: USDOE

OSTI ID:: 1982570

Journal Information:: Monthly Notices of the Royal Astronomical Society, Journal Name: Monthly Notices of the Royal Astronomical Society Journal Issue: 2 Vol. 511; ISSN 0035-8711

Publisher:: Oxford University PressCopyright Statement

Country of Publication:: United States

Language:: English

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79 ASTRONOMY AND ASTROPHYSICS
Astronomy
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Function
Galaxies
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Mass function
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The dark matter haloes of HI selected galaxies

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