Analysis of the oscillations in HST observations of the quiescent SU UMa type dwarf nova WZ Sagittae
Cyclical period changes in the dwarf novae V2051 Oph and V4140 Sgr
HST and ground-based eclipse observations of V2051 Ophiuchi: binary parameters
Hubble Space Telescope Faint Object Spectrograph Spectral Mapping of V2051 Ophiuchi in a Low State
Two new systems with enhanced UV line flux ratios as indication of the evolution of cataclysmic variables
Instrument
FOS/BL, FOS/RD, HRS/2
Temporal Coverage
1995-10-24T04:34:19Z/1996-03-20T06:56:14Z
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, Horne comma Keith, 1997, 'SUPERSONIC VELOCITY DISPERSION IN DWARF NOVA ACCRETION DISKS', 1.0, European Space Agency, https://doi.org/10.5270/esa-a4dac3z