On the late spectral types of cataclysmic variable secondaries
- 1 October 2000
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 318 (2) , 354-360
- https://doi.org/10.1046/j.1365-8711.2000.t01-1-03628.x
Abstract
No abstract availableKeywords
This publication has 22 references indexed in Scilit:
- Brown dwarfs and the cataclysmic variable period minimumMonthly Notices of the Royal Astronomical Society, 1999
- The NextGen Model Atmosphere Grid for 3000 ≤ Teff ≤ 10,000 KThe Astrophysical Journal, 1999
- MODEL ATMOSPHERES OF VERY LOW MASS STARS AND BROWN DWARFSAnnual Review of Astronomy and Astrophysics, 1997
- New Evolutionary Tracks for Very Low Mass StarsThe Astrophysical Journal, 1995
- The derived population of luminous supersoft X-ray sourcesThe Astrophysical Journal, 1994
- The initial periods of cataclysmic variables and the maximum field strength in AM-Herculis systemsMonthly Notices of the Royal Astronomical Society, 1994
- An expanded set of brown dwarf and very low mass star modelsThe Astrophysical Journal, 1993
- Magnetic braking and the evolution of cataclysmic binariesMonthly Notices of the Royal Astronomical Society, 1988
- Calculated gamma-ray line fluxes from the Type II supernova 1987 AThe Astrophysical Journal, 1987
- Radio emission from the nova-like variable AC CANCRI and the symbiotic variable AG DraconisThe Astrophysical Journal, 1987