Absorption by Highly Ionized Interstellar Gas Along Extragalactic and Galactic Sight Lines
Complex X-Ray Absorption and the Fe Ka Profile in NGC 3516
Evolution of the Outflows in NGC 3516
Intrinsic Absorption Lines in Seyfert 1 Galaxies. I. Ultraviolet Spectra from the Hubble Space Telescope
Intrinsic absorption with the Far Ultraviolet Spectroscopic Explorer
Resolving the Intrinsic C IV Absorption in the Seyfert 1 Galaxy NGC 3516
Variable Ultraviolet Absorption in the Seyfert 1 Galaxy NGC 3516: The Case for Associated Ultraviolet and X-Ray Absorption
Instrument
HRS, HRS/2
Temporal Coverage
1995-04-24T21:44:05Z/1995-04-25T08:57:49Z
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, Maran comma Stephen P., 1996, 'ABSORPTION CLOUD PHYSICS IN SEYFERT GALAXY NUCLEI -- CYCLE 2', 1.0, European Space Agency, https://doi.org/10.5270/esa-ywrnplm