Cloud-by-cloud multiphase investigation of the circumgalactic medium of low-redshift galaxies
Halo Mass Dependence of H I and O VI Absorption: Evidence for Differential Kinematics
Kinematics of the O VI Circumgalactic Medium: Halo Mass Dependence and Outflow Signatures
The Azimuthal Dependence of Outflows and Accretion Detected Using O VI Absorption
The Highly Ionized Circumgalactic Medium is Kinematically Uniform around Galaxies
The Relation between Galaxy ISM and Circumgalactic O VI Gas Kinematics Derived from Observations and LCDM Simulations
Instrument
COS, COS/FUV, COS/NUV
Temporal Coverage
2011-02-19T17:35:54Z/2011-05-27T07:58:27Z
Version
1.0
Mission Description
Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
European Space Agency, Churchill et al., 2013, 'The Relative Kinematics of Galaxy Emission and Multiple Gas Phases in z~0.5 Extended Galaxy Halos', 1.0, European Space Agency, https://doi.org/10.5270/esa-d8domtn