The product of the globular cluster collapse

Details The product of the globular cluster collapse The product of the globular cluster collapse

Aug 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ap%26ss.194..131z&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 194, no. 1, p. 131-142.

Statistics

Computation

Binary Stars, Black Holes (Astronomy), Globular Clusters, Gravitational Collapse, Stellar Evolution, Computational Astrophysics, Stellar Mass, X Ray Sources

Scientific paper

In this paper we calculate the number of close binaries formed during the evolution process of a globular cluster core. The globular cluster core is assumed to contain a massive black hole at its center. We show that the central black hole can drive binary formation in the core and the rate of binary formation depends on the mass of the black hole at its center. Whether cluster X-ray is produced mainly by the central black hole or by binaries in the core depends on the mass of the central black hole. Therefore, two cases arise: black hole accretion domination, and binary radiation domination. The possibility of the existence of a central black hole exists even when binary radiation characteristics have been observed in globular cluster X-ray sources.

Affiliated with

Also associated with

No associations

Rating

The product of the globular cluster collapse 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 The product of the globular cluster collapse, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The product of the globular cluster collapse will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1165553