Irradiation-driven mass transfer in low-mass X-ray binaries
- 1 March 1991
- journal article
- Published by Springer Nature in Nature
- Vol. 350 (6314) , 136-138
- https://doi.org/10.1038/350136a0
Abstract
No abstract availableKeywords
This publication has 11 references indexed in Scilit:
- Genesis of pulsars in globular clustersNature, 1990
- Late evolution of very low mass X-ray binaries sustained by radiation from their primariesThe Astrophysical Journal, 1989
- The evolution of irradiated starsMonthly Notices of the Royal Astronomical Society, 1989
- Accretion turnoff and rapid evaporation of very light secondaries in low-mass X-ray binariesThe Astrophysical Journal, 1989
- Photometry and the light curve of the optical counterpart of the eclipsing millisecond pulsar 1957+20The Astrophysical Journal, 1988
- Spectroscopy of the M15 X-ray source: discovery of binary motion and an unusual systemic velocityMonthly Notices of the Royal Astronomical Society, 1988
- A new technique for calculations of binary stellar evolution, with application to magnetic brakingThe Astrophysical Journal, 1983
- On the evolutionary status of bright, low-mass X-ray sourcesThe Astrophysical Journal, 1983
- Dynamical Instabilities and Mass Exchange in Binary SystemsMonthly Notices of the Royal Astronomical Society, 1975
- Self-Excited Flow in Binary X-Ray SourcesThe Astrophysical Journal, 1973