Characterizing Transition Temperature Gas in the Galactic Corona
Chasing obscuration in type-I AGN: discovery of an eclipsing clumpy wind at the outer broad-line region of NGC 3783
HST/COS observations of the newly discovered obscuring outflow in NGC 3783
Measuring Turbulence in the Interstellar Medium by Comparing N(H I; Lya) and N(H I; 21 cm)
New Constraints on the Nature and Origin of the Leading Arm of the Magellanic Stream
The Ionized Gas and Nuclear Environment in NGC 3783. II. Averaged Hubble Space Telescope/STIS and Far Ultraviolet Spectroscopic Explorer Spectra
The Ionized Gas and Nuclear Environment in NGC 3783. III. Detection of a Decreasing Radial Velocity in an Intrinsic Ultraviolet Absorber
The Ionized Gas and Nuclear Environment in NGC 3783. V. Variability and Modeling of the Intrinsic Ultraviolet Absorption
The Milky Way halo as a QSO absorption-line system. New results from an HST/STIS absorption-line catalogue of Galactic high-velocity clouds
Toward a Self-Consistent Model of the Ionized Absorber in NGC 3783
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
2000-08-05T00:48:21Z/2002-01-06T16:00:51Z
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, Crenshaw comma D. Michael, 2007, 'Determining the Nature of the Variable Absorption in AGN: Monitoring NGC 3783 with HST and Chandra', 1.0, European Space Agency, https://doi.org/10.5270/esa-va9nksr