Constraining the evolution of cataclysmic variables via the masses and accretion rates of their underlying white dwarfs
Early and Extended Helium Reionization over More Than 600 Million Years of Cosmic Time
Effective temperatures of cataclysmic-variable white dwarfs as a probe of their evolution
Evidence for mass accretion driven by spiral shocks onto the white dwarf in SDSS J123813.73-033933.0
Evolution of spin in the intermediate polar CC sculptoris
GW Lib: a Unique Laboratory for White Dwarf Pulsations
GW Librae: a unique laboratory for pulsations in an accreting white dwarf
GW Librae: Still Hot Eight Years Post-outburst
Helium Reionization Simulations. III. The Helium Lya Forest
Hubble COS Spectroscopy of the Dwarf Nova CW Mon: The White Dwarf in Quiescence?
Hubble Space Telescope Ultraviolet Light Curves Reveal Interesting Properties of CC Sculptoris and RZ Leonis
Spectroscopy from the Hubble Space Telescope Cosmic Origins Spectrograph of the Southern Nova-like BB Doradus in an Intermediate State
The C/N ratio from FUV spectroscopy as a constraint on evolution of the dwarf nova HS 0218 + 3229
White Dwarf Photospheric Abundances in Cataclysmic Variables. III. Five Dwarf Novae with an Evolved Secondary Donor Star
White Dwarf Photospheric Abundances in Cataclysmic Variables-II. White Dwarfs with and without a Mask
XMM-Newton observations of the low-luminosity cataclysmic variable V405 Pegasi
Instrument
COS, COS/FUV, COS/NUV
Temporal Coverage
2012-10-12T01:17:07Z/2014-03-20T14:10:37Z
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, Gaensicke et al., 2014, 'The mass and temperature distribution of accreting white dwarfs', 1.0, European Space Agency, https://doi.org/10.5270/esa-ylww2tz