On the Properties of Galactic Novae and Their Orbital Period Distribution
- 20 February 2004
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 602 (2), 938-947
- https://doi.org/10.1086/381156
Abstract
No abstract availableThis publication has 39 references indexed in Scilit:
- On the formation of oxygen-neon white dwarfs in close binary systemsAstronomy & Astrophysics, 2001
- An Exploration of the Paradigm for the 2–3 Hour Period Gap in Cataclysmic VariablesThe Astrophysical Journal, 2001
- Multiwavelength Superoutburst Observations of T LeonisPublications of the Astronomical Society of the Pacific, 1999
- LUMINOUS SUPERSOFT X-RAY SOURCESAnnual Review of Astronomy and Astrophysics, 1997
- On the existence of low-luminosity cataclysmic variables beyond the orbital period minimumMonthly Notices of the Royal Astronomical Society, 1997
- Predictions of a population of cataclysmic variables in globular clustersThe Astrophysical Journal, 1994
- The nova rate in the elliptical component of NGC 5128The Astronomical Journal, 1990
- Magnetic braking and the evolution of cataclysmic binariesMonthly Notices of the Royal Astronomical Society, 1988
- Hot accreting white dwarfs in the quasi-static approximationThe Astrophysical Journal, 1982
- Binaries among B2-B5 IV, V absorption and emission starsThe Astrophysical Journal Supplement Series, 1978