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
Reporting a deficit of intrinsic N V absorbers in core-dominated radio-loud quasars
Signatures of gas flows - I. Connecting the kinematics of the H I circumgalactic medium to galaxy rotation
Signatures of gas flows - II. Connecting the kinematics of the multiphase circumgalactic medium to galaxy rotation
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
2011-02-19T21:36:53Z/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, 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
Rights
Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.