A Method for Deriving Accurate Gas-Phase Abundances for the Multiphase Interstellar Galactic Halo
A Reservoir of Ionized Gas in the Galactic Halo to Sustain Star Formation in the Milky Way
FUSE, STIS and Keck spectroscopic analysis of the UV-bright star vZ 1128 in M3 (NGC 5272)
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
Ionized Gas in the First 10 kpc of the Interstellar Galactic Halo: Metal Ion Fractions
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA, STIS/NUV-MAMA
Temporal Coverage
2002-08-16T16:34:40Z/2002-08-17T23:48:52Z
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, Howk et al., 2003, 'Understanding the Warm Ionized Medium of the Galactic Halo', 1.0, European Space Agency, https://doi.org/10.5270/esa-vuwydv4