A 110 MG cyclotron harmonic in the optical spectrum of RX J1554.2+2721
A 150 MG Magnetic White Dwarf in the Cataclysmic Variable RX J1554.2+2721
A Far Ultraviolet Archival Study of Cataclysmic Variables. I. FUSE and HST STIS Spectra of the Exposed White Dwarf in Dwarf Nova Systems
A Far-Ultraviolet Spectroscopic Analysis of BZ Ursae Majoris
An archive study of 18 old novae. I. The UV spectra
An Illustration of Modeling Cataclysmic Variables: HST, FUSE, and SDSS Spectra of SDSS J080908.39+381406.2
Anomalous Ultraviolet Line Flux Ratios in the Cataclysmic Variables 1RXS J232953.9+062814, CE 315, BZ Ursae Majoris, and EY Cygni, Observed with the Hubble Space Telescope Space Telescope Imaging Spectrograph
A Statistical Study of Accretion Disk Model Spectra for Cataclysmic Variables
Composite Accretion Disk and White Dwarf Photosphere Analyses of the FUSE and Hubble Space Telescope Observations of EY Cygni
Effective temperatures of cataclysmic-variable white dwarfs as a probe of their evolution
Far-Ultraviolet Spectroscopy of Magnetic Cataclysmic Variables
HS 2331+3905: The cataclysmic variable that has it all
Hubble Space Telescope and Ground-based Observations of V455 Andromedae Post-outburst
Hubble Space Telescope STIS Spectroscopy of Long-Period Dwarf Novae in Quiescence
Hubble Space Telescope STIS Spectroscopy of Nova T Aurigae 1891
Hubble Space Telescope STIS Spectroscopy of the Peculiar Nova-Like Variables BK Lyn, V751 Cygni, and V380 Oph
MV Lyrae in Low, Intermediate, and High States
Observational studies of Cataclysmic Variable evolution: Of samples, biases and surprises
SWSextantis stars: the dominant population of cataclysmic variables with orbital periods between 3 and 4h
The Accreting, Pulsating White Dwarfs in Cataclysmic Variables
The Accreting White Dwarfs in Cataclysmic Variables
The instability strip for accreting pulsating white dwarfs as a probe for accretion heating/cooling .
Time-resolved photometry and spectroscopy of the new deeply-eclipsing SW Sextantis star HS 0728+6738
Two new systems with enhanced UV line flux ratios as indication of the evolution of cataclysmic variables
Ultraviolet spectroscopic investigation of HU Aqr and AN UMa with the data from HST and IUE
Ultraviolet spectroscopic study of EU UMa and ST LMi from HST and IUE observations
White Dwarf Photospheric Abundances in Cataclysmic Variables. III. Five Dwarf Novae with an Evolved Secondary Donor Star
White Dwarf Photospheric Abundances in Cataclysmic Variables. I. SS Aurigae and TU Mensae
White dwarfs in cataclysmic variable stars: accretion physics and evolution.
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
2002-10-11T20:33:53Z/2003-07-06T06:05:24Z
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 comma Boris T., 2003, 'Towards a global understanding of accretion physics --, Clues from an UV spectroscopic survey of cataclysmic variables', 1.0, European Space Agency, https://doi.org/10.5270/esa-eoc1kkw
