An HST/COS legacy survey of high-velocity ultraviolet absorption in the Milky Ways circumgalactic medium and the Local Group
A population of high-velocity absorption-line systems residing in the Local Group
A Reservoir of Ionized Gas in the Galactic Halo to Sustain Star Formation in the Milky Way
Deep Herschel view of obscured star formation in the Bullet cluster
Evidence for a Massive, Extended Circumgalactic Medium Around the Andromeda Galaxy
Intermediate- and high-velocity clouds in the Milky Way - I. Covering factors and vertical heights
Intermediate- and high-velocity clouds in the Milky Way - II. Evidence for a Galactic fountain with collimated outflows and diffuse inflows
Origin(s) of the Highly Ionized High-Velocity Clouds Based on Their Distances
Instrument
COS, COS/FUV, STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
2009-10-06T05:52:46Z/2010-11-28T17:39:12Z
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, Lehner comma Nicolas, 2011, 'Testing the Origin{s} of the Highly Ionized High-Velocity Clouds: A Survey of Galactic Halo Stars at z>3 kpc', 1.0, European Space Agency, https://doi.org/10.5270/esa-h3l0fom