Abundance of Elements beyond the Iron Group in Cool DO White Dwarfs
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
Search for trans-iron elements in hot, helium-rich white dwarfs with the HST Cosmic Origins Spectrograph
Stellar laboratories: new Ge V and Ge VI oscillator strengths and their validation in the hot white dwarf RE 0503-289
The discovery of photospheric nickel in the hot DO white dwarf REJ 0503-289
Instrument
HRS, HRS/2
Temporal Coverage
1996-09-03T15:54:10Z/1997-01-22T05:04:31Z
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, Werner et al., 1998, 'METAL DIFFUSION AND RADIATIVE LEVITATION IN HOT HELIUM-RICH WHITE DWARFS', 1.0, European Space Agency, https://doi.org/10.5270/esa-tnsuwef