Exploding neutron stars in close binaries

Details Exploding neutron stars in close binaries Exploding neutron stars in close binaries

Jun 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984pazh...10..422b&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 10, June 1984, p. 422-428) Soviet Astronomy Letters (ISSN 0360-0327), vol. 10, May-June

Astronomy and Astrophysics

Astronomy

40

Binary Stars, Black Holes (Astronomy), Neutron Stars, Star Clusters, Stellar Evolution, Gravitational Waves, Hubble Constant

Scientific paper

The evolution of a close binary system consisting of a neutron star and a black hole or another neutron star is considered. It is shown that the matter outflow from the neutron star results in quasi-static evolution of the star until the state of minimum possible mass mmin ≈ 0.09 M_sun; and the following explosion. In compact stellar clusters or galactic nuclei the total time of the process leading to explosion is less than the Hubble time.

Affiliated with

Also associated with

No associations

Rating

Exploding neutron stars in close 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 Exploding neutron stars in close binaries, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Exploding neutron stars in close binaries will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1855730