The Multiphase Intracluster Medium in Galaxy Groups Probed by the Lyman Alpha Forest

Abstract

The case is made that the intracluster medium (ICM) in spiral-rich galaxy groups today probably has undergone much slower evolution than that in elliptical-rich groups and clusters. The environments of proto-clusters and proto-groups at z > 2 are likely similar to spiral-rich group environments at lower redshift. Therefore, like the ICM in spiral-rich groups today, the ICM in proto-groups and proto-clusters at z > 2 is predicted to be significantly multiphased. The QSO Lyman alpha forest in the vicinity of galaxies is an effective probe of the ICM at a wide range of redshift. Two recent observations of Lyman alpha absorption around galaxies by Adelberger et al. and by Pascarelle et al are reconciled, and it is shown that observations support the multiphase ICM scenario. Galaxy redshifts must be very accurate for such studies to succeed. This scenario can also explain the lower metallicity and lower hot gas fraction in groups.

4 pages, 1 figure, replaced with the version after proof

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Cited by in corpus (4)

• Thick disks and halos of spiral galaxies M 81, NGC 55 and NGC 300
• HI in the proto-cluster environment at z>2: absorbing haloes and the Lyman alpha forest
• The velocity field of baryonic gas in the universe
• Low-Metallicity Gas Clouds in a Galaxy Proto-Cluster at Redshift 2.38