CGM2 I: The Extent of the Circumgalactic Medium Traced by Neutral Hydrogen
We present initial results from the Cosmic Origins Spectrograph (COS) and Gemini Mapping the Circumgalactic Medium (CGMCGM ≡ CGM2) survey. The CGM2 survey consists of 1689 galaxies, all with high-quality Gemini-GMOS spectra, within 1 Mpc of 22 z ≲ 1 quasars, all with a signal-to-noise ratio of ∼10 H...
Saved in:
Published in | The Astrophysical journal Vol. 912; no. 1 |
---|---|
Main Authors | , , , , , , , , , , |
Format | Journal Article |
Language | English |
Published |
Philadelphia
The American Astronomical Society
01.05.2021
IOP Publishing |
Subjects | |
Online Access | Get full text |
Cover
Loading…
Summary: | We present initial results from the Cosmic Origins Spectrograph (COS) and Gemini Mapping the Circumgalactic Medium (CGMCGM ≡ CGM2) survey. The CGM2 survey consists of 1689 galaxies, all with high-quality Gemini-GMOS spectra, within 1 Mpc of 22 z ≲ 1 quasars, all with a signal-to-noise ratio of ∼10 Hubble Space Telescope/COS G130M+G160M spectra. For 572 of these galaxies with stellar masses 107 M ⊙ < M ⋆ < 1011 M ⊙ and z ≲ 0.5, we show that the H i covering fraction above a threshold of N HI > 1014cm−2 is ≳0.5 within 1.5 virial radii (R vir ∼ R 200m). We examine the H i kinematics and find that the majority of absorption lies within ±250 km s−1 of the galaxy systemic velocity. We examine H i covering fractions over a range of impact parameters to infer a characteristic size of the CGM, \({R}_{\mathrm{CGM}}^{14}\), as a function of galaxy mass. \({R}_{\mathrm{CGM}}^{14}\) is the impact parameter at which the probability of observing an absorber with N HI >1014 cm−2 is >50%. In this framework, the radial extent of the CGM of M ⋆ > 109.9 M ⊙ galaxies is \({R}_{\mathrm{CGM}}^{14}={346}_{-53}^{+57}\) kpc or \({R}_{\mathrm{CGM}}^{14}\simeq 1.2{R}_{\mathrm{vir}}\). Intermediate-mass galaxies with 109.2 < M ⋆/M ⊙ < 109.9 have an extent of \({R}_{\mathrm{CGM}}^{14}={353}_{-50}^{+64}\) kpc or \({R}_{\mathrm{CGM}}^{14}\simeq 2.4{R}_{\mathrm{vir}}\). Low-mass galaxies, M ⋆ < 109.2 M ⊙, show a smaller physical scale of \({R}_{\mathrm{CGM}}^{14}={177}_{-65}^{+70}\) kpc and extend to \({R}_{\mathrm{CGM}}^{14}\simeq 1.6{R}_{\mathrm{vir}}\). Our analysis suggests that using R vir as a proxy for the characteristic radius of the CGM likely underestimates its extent. |
---|---|
Bibliography: | Galaxies and Cosmology AAS26627 |
ISSN: | 0004-637X 1538-4357 |
DOI: | 10.3847/1538-4357/abea14 |