HST Spectroscopy of PG 1159 Stars: the Boundary of the GW VIR Instability Strip
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
Spectral analyses of PG 1159 star: constraints on the GW Virginis pulsations from HST observations
The far-ultraviolet spectra of cool PG 1159 stars
UV Spectroscopy of Hydrogen-Deficient Post-AGB Stars: PG 1144+005 and PG 1520+525
Instrument
HRS, HRS/1
Temporal Coverage
1995-08-02T07:00:00Z/1995-09-22T02:59:46Z
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, Heber et al., 1996, 'NLTE SPECTRAL ANALYSIS OF PG1159 STARS: FINDING THE LIMITS OF THE GW VIR INSTABILITY STRIP', 1.0, European Space Agency, https://doi.org/10.5270/esa-kp8oha8