Aperture and Resolution Effects on Ultraviolet Star-forming Properties: Insights from Local Galaxies and Implications for High-redshift Observations
A robust measurement of the mass outflow rate of the galactic outflow from NGC 6090
Far-ultraviolet Observations of Outflows from Infrared-luminous Galaxies
Metal-enriched galactic outflows shape the mass-metallicity relationship
Scaling Relations Between Warm Galactic Outflows and Their Host Galaxies
Shining a light on galactic outflows: photoionized outflows
Supernova-driven outflows in NGC 7552: a comparison of H a and UV tracers
Synthetic Absorption Lines from Simulations of Multiphase Gas in Galactic Winds
The Magellan Evolution of Galaxies Spectroscopic and Ultraviolet Reference Atlas (MegaSaura). II. Stacked Spectra
The mass and momentum outflow rates of photoionized galactic outflows
Instrument
COS, COS/FUV, COS/NUV
Temporal Coverage
2011-05-10T21:25:15Z/2011-10-21T23:10:56Z
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, Leitherer et al., 2012, 'Feedback between Stars, ISM and IGM in IR-Luminous Galaxies', 1.0, European Space Agency, https://doi.org/10.5270/esa-icyv2gz