On the formation rate of close binaries consisting of a super-massive black hole and a white dwarf
Open Access
- 21 October 2002
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 336 (2) , 373-381
- https://doi.org/10.1046/j.1365-8711.2002.05733.x
Abstract
No abstract availableKeywords
All Related Versions
This publication has 10 references indexed in Scilit:
- The Distribution of Stars near the Supermassive Black Hole in the Galactic CenterThe Astrophysical Journal, 1999
- Black Hole PhysicsFundamental Theories of Physics, 1998
- Capture of stellar mass compact objects by massive black holes in galactic cuspsMonthly Notices of the Royal Astronomical Society, 1997
- Gradual approach to coalescence for compact stars orbiting massive black holesThe Astrophysical Journal, 1995
- Numerical models of star clusters with a central black hole. I - Adiabatic modelsThe Astrophysical Journal, 1980
- The stellar distribution around a black hole - Numerical integration of the Fokker-Planck equationThe Astrophysical Journal, 1978
- Star clusters containing massive, central black holes - Monte Carlo simulations in two-dimensional phase spaceThe Astrophysical Journal, 1978
- The distribution and consumption rate of stars around a massive, collapsed objectThe Astrophysical Journal, 1977
- Star distribution around a massive black hole in a globular clusterThe Astrophysical Journal, 1976
- Star Distribution Near a Collapsed ObjectThe Astrophysical Journal, 1972