A Comparative Study of the Atmospheric Composition of the DA White Dwarfs Feige 24 and G191-B2B
A photospheric metal line profile analysis of hot DA white dwarfs with circumstellar material
Circumstellar features in hot DA white dwarfs
Discovery of Photospheric Germanium in Hot DA White Dwarfs
Heavy-element abundance patterns in hot DA white dwarfs
Hubble Space Telescope Imaging Spectrograph Observations of the Hot White Dwarf in the Close Binary Feige 24
Orbital Parameters and Chemical Composition of Four White Dwarfs in Post-Common-Envelope Binaries
The origin of hot white dwarf circumstellar features
The Structure of the Local Interstellar Medium. V. Electron Densities
Two New Low Galactic D/H Measurements from the Far Ultraviolet Spectroscopic Explorer
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
1997-11-29T10:28:46Z/1998-01-04T10:16:32Z
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, Vennes comma Stephane, 1999, 'Fundamental Parameters of White Dwarfs in Close Binaries with Late-Type Stars', 1.0, European Space Agency, https://doi.org/10.5270/esa-9sg36tm