Black holes in X-ray binary systems - Observational data and evolutionary status

Details Black holes in X-ray binary systems - Observational data and evolutionary status Black holes in X-ray binary systems - Observational data and evolutionary status

Jun 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997azh....74..407t&link_type=abstract

Astronomicheskij Zhurnal, vol. 74, p. 407

Astronomy and Astrophysics

Astronomy

4

X Ray Binaries, Black Holes (Astronomy), Stellar Evolution, Light Curve, Relativity, Roche Limit, O Stars, B Stars

Scientific paper

We analyze the main parameters, that are significant from the standpoint of evolution, of the ten most reliably observed black-hole candidates among the components of close X-ray binary systems. The principal driving forces of the evolution of these systems can be established by analyzing their evolution. These are induced (in binaries with F-M donors) and self-induced (in binaries with O-B donors) stellar winds from donors that almost fill their Roche lobes. The driving force of the evolution of V404 Cyg, XN Oph, and XN Sco is probably evolutionary expansion of the donors, a solar-mass star with a degenerate helium core. The space velocities of X-ray binaries with black holes can be explained in terms of the recoil effect produced by supernova explosions in close binary systems.

Affiliated with

Also associated with

No associations

Rating

Black holes in X-ray binary systems - Observational data and evolutionary status 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 holes in X-ray binary systems - Observational data and evolutionary status, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Black holes in X-ray binary systems - Observational data and evolutionary status will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1473382