%0 Generic %1 bielby2016probing %A Bielby, R. %A Crighton, N. H. M. %A Fumagalli, M. %A Morris, S. L. %A Stott, J. P. %A Tejos, N. %A Cantalupo, S. %D 2016 %K absorption group medium %T Probing the intra-group medium of a z = 0.28 galaxy group %U http://arxiv.org/abs/1607.03386 %X We present new MUSE observations of a galaxy group probed by a background quasar. The quasar sightline passes between multiple $z=0.28$ galaxies, whilst showing at the same redshift low ionised metal line species, including Ca II, Mg I, Mg II and Fe II. Based on the galaxy redshifts measured from the MUSE data, we estimate the galaxies to be part of a small galaxy group with a halo mass of $\approx6\times10^12$ M$_ødot$. We use the MUSE data to reveal the two dimensional dynamical properties of the gas and stars in the group galaxies, and relate these to the absorber kinematics. With these data we consider four scenarios for the nature of the gas probed by the sightline absorbers: a co-rotating gas halo associated with a single galaxy within the group; outflowing material from a single group member powered by recent star-formation; and cool dense gas embedded within the intra-group medium. We find that the dynamics, alongside the galaxy impact parameters and star-formation rates, favour the latter, in which the cool gas belongs to the intra-group medium and is likely pressure confined within a warmer gas halo.

@misc{bielby2016probing, abstract = {We present new MUSE observations of a galaxy group probed by a background quasar. The quasar sightline passes between multiple $z=0.28$ galaxies, whilst showing at the same redshift low ionised metal line species, including Ca II, Mg I, Mg II and Fe II. Based on the galaxy redshifts measured from the MUSE data, we estimate the galaxies to be part of a small galaxy group with a halo mass of $\approx6\times10^{12}$ M$_{\odot}$. We use the MUSE data to reveal the two dimensional dynamical properties of the gas and stars in the group galaxies, and relate these to the absorber kinematics. With these data we consider four scenarios for the nature of the gas probed by the sightline absorbers: a co-rotating gas halo associated with a single galaxy within the group; outflowing material from a single group member powered by recent star-formation; and cool dense gas embedded within the intra-group medium. We find that the dynamics, alongside the galaxy impact parameters and star-formation rates, favour the latter, in which the cool gas belongs to the intra-group medium and is likely pressure confined within a warmer gas halo.}, added-at = {2016-07-13T10:12:41.000+0200}, author = {Bielby, R. and Crighton, N. H. M. and Fumagalli, M. and Morris, S. L. and Stott, J. P. and Tejos, N. and Cantalupo, S.}, biburl = {https://www.bibsonomy.org/bibtex/2223651ef1198032ba4d70cce7a700065/miki}, description = {[1607.03386] Probing the intra-group medium of a z = 0.28 galaxy group}, interhash = {5a53646fa5eb0c3d787fbfccea237db4}, intrahash = {223651ef1198032ba4d70cce7a700065}, keywords = {absorption group medium}, note = {cite arxiv:1607.03386Comment: 14 pages, 9 figures, submitted to MNRAS}, timestamp = {2016-07-13T10:12:41.000+0200}, title = {Probing the intra-group medium of a z = 0.28 galaxy group}, url = {http://arxiv.org/abs/1607.03386}, year = 2016 }