Adding More Mysteries to the DA White Dwarf GD 394
Analysis of Optical and Ultraviolet Spectroscopy of the DAZ White Dwarf G74-7
Analysis of UV and optical spectra of the helium-rich white dwarfs HS 2253+8023 and GD 40
Circumstellar features in hot DA white dwarfs
Element abundances in cool white dwarfs. I. The DZA white dwarfs L 745-46A and Ross 640
Far-UV spectroscopy of two extremely hot, helium-rich white dwarfs
Heavy-element abundance patterns in hot DA white dwarfs
High ions towards white dwarfs: circumstellar line shifts and stellar temperature
Hubble Space Telescope Observations of Cool White Dwarf Stars: Detection of New Species of Heavy Elements
Hubble Space Telescope observations of white dwarfs in detached binaries
Hubble Space Telescope spectroscopy of hot helium-rich white dwarfs: metal abundances along the cooling sequence
Iron abundance in hot hydrogen-deficient central stars and white dwarfs from FUSE, HST, and IUE spectroscopy
Line shapes of the magnesium resonance lines in cool DZ white dwarf atmospheres
Photospheric, Circumstellar, and Interstellar Features of HE, C, O, and SI in the HST Spectra of Four Hot White Dwarf Stars
Solving the mystery of the heavy-element opacity in the DA white dwarf GD 394.
Spectral analysis of the hot DO white dwarf PG1034+001.
The origin of hot white dwarf circumstellar features
Variations in D/H and D/O from New Far Ultraviolet Spectroscopic Explorer Observations
Instrument
FOS/BL, FOS/RD, HRS, HRS/2, WFPC/WFC
Temporal Coverage
1992-06-05T07:39:01Z/1992-09-13T03:49:47Z
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.
