Physics
Scientific paper
Apr 1999
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999phr...311..337k&link_type=abstract
Physics Reports, Vol. 311, No. 3 - 5, p. 337 - 344
Physics
4
X-Ray Binaries: Transients, X-Ray Binaries: Black Holes, X-Ray Binaries: Neutron Stars
Scientific paper
The appearance of transient behaviour in a low-mass X-ray binary places very strong constraints on the system. These are most easily satisfied if the accretor is a black hole, as in this case the system cannot easily attain a persistent state in which the central accretor keeps the accretion disc ionized and therefore stable by irradiating it. In contrast, neutron star systems can only become transient if the companion star is already evolved before mass transfer starts. Formation constraints actually mean that this requirement is, nevertheless, fulfilled in a significant fraction of neutron-star systems. The outburst light curves of both types of transient are dominated by irradiation. Propagation of the cooling wave that terminates dwarf nova outbursts is thus prevented in transient discs until most of the disc mass has been accreted, accounting for their long duration, shape, and long recurrence time.
No associations
LandOfFree
Black hole and transient binaries. does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Black hole and transient binaries., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Black hole and transient binaries. will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-893998