Discovery of a Primitive Damped Lyα Absorber near an X‐Ray–bright Galaxy Group in the Virgo Cluster

Abstract

We present a new ultraviolet echelle spectrum of PG 1216+069, obtained with the Space Telescope Imaging Spectrograph on board the Hubble Space Telescope, that reveals damped Lyabsorption, as well as O i ,C ii ,S iii, and Fe iiabsorption lines, at zabs ¼ 0:00632 near the NGC 4261 galaxy group in the periphery of the Virgo Cluster. Theabsorbershowsnoevidenceofhighlyionizedgas,whichplacesconstraintson''warm-hot''missingbaryonsin the X-ray-bright NGC 4261 group. The well-developed damping wings of the Lyline tightly constrain the H i columndensity;wefindlogN(Hi) ¼ 19:32 � 0:03.ThemetallicityofthissubdampedLyabsorber(sub-DLA) is remarkably low, ½O=H �¼� 1:60 þ0:09 � 0:11 , comparable to many analogous high-redshift systems, and the iron abun- dance indicates that this absorber contains little or no dust. Nitrogen is underabundant: we detect neither N i nor N ii, and we show that the absence of nitrogen is not due to ionization effects but rather indicates that ½N=O �� � 0:28 (3 � ). Despite the proximity of the sight line to the NGC 4261 group, there are no bright galaxies with small impact parameters at the absorption redshift: the nearest known galaxy is a sub-L* galaxy with a projected distance of � ¼ 86 h � 1 75 kpc, while the closest L *g alaxy is NGC 4260, at� ¼ 246 h � 1 75 kpc. The low metallicity and ni- trogen underabundance indicate that this low-z sub-DLA is a relatively primitive gas cloud. We consider the na- ture and origin of the sub-DLA, and we discuss several possibilities. The properties of the sub-DLA are similar to those of the interstellar media in blue compact dwarf galaxies and are also reminiscent of Milky Way high-velocity clouds. The sub-DLA could also be related to a dwarf spheroidal galaxy, if the absorption arises in gas ejected or stripped from such an object. Finally, the object could simply be a small dark matter halo, self-enriched by a small amount of internal star formation but mostly undisturbed since its initial formation. In this case, the small halo would likely be an ancient building block of galaxy formation that formed before the epoch of reionization. Subject headingg cosmology: observations — galaxies: abundances — intergalactic medium — quasars: absorption lines — quasars: individual (PG 1216+069)