Changes and Absorption Features in the Ultraviolet Spectrum of the PG 1159-Type Central Star RX J2117+3412
High ions towards white dwarfs: circumstellar line shifts and stellar temperature
High resolution UV spectroscopy of two hot (pre-) white dwarfs with the Hubble Space Telescope. KPD0005+5106 and RXJ2117+3412.
Identification of Ne VIII lines in H-deficient (pre-) white dwarfs: a new tool to constrain the temperature of the hottest stars
Iron abundance in hot hydrogen-deficient central stars and white dwarfs from FUSE, HST, and IUE spectroscopy
M31s Heavy-Element Distribution and Outer Disk
Metal abundances in the hottest known DO white dwarf (KPD 0005+5106)
Instrument
HRS, HRS/2
Temporal Coverage
1994-05-31T20:54:53Z/1994-06-01T05:31:26Z
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 comma Klaus, 1995, 'ORIGIN OF THE ULTRAHIGH-IONISATION OVIII EMISSION LINES IN TWO EXCEP- TIONAL (PRE-)WHITE DWARFS: KPD0005+5106 AND RXJ2117+3412: CYCLE4 HIGH', 1.0, European Space Agency, https://doi.org/10.5270/esa-swzs2d3