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(1 - 8 of 8)
Low-mass group environments have no substantial impact on the circumgalactic medium metallicity
The Relationship between Galaxy ISM and Circumgalactic Gas Metallicities
Kinematics of the O VI Circumgalactic Medium: Halo Mass Dependence and Outflow Signatures
Relationship between the Metallicity of the Circumgalactic Medium and Galaxy Orientation
The Relation between Galaxy ISM and Circumgalactic O VI Gas Kinematics Derived from Observations and ΛCDM Simulations
Understanding the strong intervening O VI absorber at z_abs 0.93 towards PG1206+459
The Highly Ionized Circumgalactic Medium is Kinematically Uniform around Galaxies
The Impact of the Group Environment on the O VI Circumgalactic Medium