A Preliminary Observational Search for Circumbinary Disks around Cataclysmic Variables
A Synthetic Spectrum and Light-Curve Analysis of the Cataclysmic Variable IX Velorum
Orbital and stochastic far-ultraviolet variability in the nova-like system V3885 Sgr
QU Car: a very high luminosity nova-like binary with a carbon-enriched companion
Resonance Line Profile Calculations Based on Hydrodynamical Models of Cataclysmic Variable Winds
Stellar Exotica in 47 Tucanae
Synthetic Spectrum Constraints on a Model of the Cataclysmic Variable QU Carinae
Testing the line-driven disc wind model: time-resolved ultraviolet spectroscopy of IX Vel and V3885Sgr
The Structure of the Local Interstellar Medium. V. Electron Densities
Time-resolved ultraviolet spectroscopy of the compact interacting binary QU Car
V3885 Sagittarius: A Comparison with a Range of Standard Model Accretion Disks
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
2000-02-12T20:18:30Z/2000-11-13T02:24:22Z
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, Drew comma Janet E., 2007, 'Cataclysmic Variable Disk Winds: a high time- and spectral resolution study of flow inhomogeneity', 1.0, European Space Agency, https://doi.org/10.5270/esa-wj9upvu