Studying the gaseous outskirts of galaxy groups with coherent Ly alpha absorption patterns

Abstract

In this study, we explore the properties of diffuse intergalactic gas residing in the outskirts of the four nearby, low-mass galaxy groups NGC1052, NGC5866, NGC4631, and NGC3992 (all at cz<2000 km/s) beyond their group virial radii. Using archival ultraviolet absorption spectra of bright AGN observed with HST/COS, we search for HI Ly a absorption near the groups' recession velocities along 35 sightlines that pass the outer group medium (OGrM) at normalized impact parameters rho/Rvir=1-3. We derive HI column densities of the absorbers and constrain the physical conditions in the gas by using a hydrostatic toy model of the groups' gas environment and assuming photoionization. HI Ly absorption near the groups' recession velocities is detected along 19 sightlines with HI column densities in the range log N(HI)=12.50-14.34, implying a high OGrM detection rate of more than 50 percent. We transform this value into an incidence rate of OGrM absorbers per unit redshift of dN/dz=232pm58.This is 25 percent above the value derived for the general population of Ly a absorbers within z = 0 filaments and more than twice the value for the z = 0 Ly a forest. From the modeling, we obtain lower limits for the gas densities from log n_H=-5.00 to -3.72, comparable to densities found in the overall Ly a forest. Our study unveils a large cross section and overdensity of Ly a absorbers in the outskirts of these four nearby groups. Such an overdensity is in line with a previously proposed scenario, in which AGN feedback lifts gaseous material to large distances beyond the virial radius of groups into the OGrM. However, a larger survey of OGrM absorbers and a comparison with hydrodynamical simulations will be necessary to constrain the cosmological mass density of OGrM absorbers and pinpoint their role in cosmological structure formation and galaxy/group evolution.

arXiv comment16 pages, 9 figures; accepted for publication in A&A

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