A photospheric metal line profile analysis of hot DA white dwarfs with circumstellar material
Circumstellar features in hot DA white dwarfs
Detection of Al II in the Ultraviolet Spectra of Metal-poor Stars: An Empirical LTE Test of NLTE Aluminum Abundance Calculations
D/H Along the Line of Sight of REJ 1738+665
Far-ultraviolet spectroscopy of the hot DA white dwarf WD 2218+706 (DeHt5) with STIS
Heavy-element abundance patterns in hot DA white dwarfs
Heavy element abundances in DAO white dwarfs measured from FUSE data
High ions towards white dwarfs: circumstellar line shifts and stellar temperature
Iron in Hot DA White Dwarfs
Spectral analysis of the extremely hot DA white dwarf PG 0948+534
The distribution of metals in hot DA white dwarfs
The origin of hot white dwarf circumstellar features
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
1999-06-25T16:57:38Z/2000-10-16T22:53:00Z
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, Barstow comma Martin, 2006, 'THE COMPOSITION AND EVOLUTION OF EXTREMELY HOT DA WHITE DWARFS', 1.0, European Space Agency, https://doi.org/10.5270/esa-t5det9m