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 Study of the Nova-like V794 Aquilae
An Illustration of Modeling Cataclysmic Variables: HST, FUSE, and SDSS Spectra of SDSS J080908.39+381406.2
A Statistical Study of Accretion Disk Model Spectra for Cataclysmic Variables
A Synthetic Spectrum and Light-Curve Analysis of the Cataclysmic Variable IX Velorum
Dwarf novae in the Hamburg quasar survey: rarer than expected
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 STIS Spectroscopy of Long-Period Dwarf Novae in Quiescence
Hubble Space Telescope STIS Spectroscopy of the Peculiar Nova-Like Variables BK Lyn, V751 Cygni, and V380 Oph
Modeling UX Ursae Majoris: An Abundance of Challenges
Two new systems with enhanced UV line flux ratios as indication of the evolution of cataclysmic variables
V3885 Sagittarius: A Comparison with a Range of Standard Model Accretion Disks
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
2003-08-17T03:20:33Z/2004-06-14T03:19:01Z
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., 2004, '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-3l4ijh3