Gravitational collapse of rotating iron-oxygen stars

Details Gravitational collapse of rotating iron-oxygen stars Gravitational collapse of rotating iron-oxygen stars

Aug 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977pazh....3..353i&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal, vol. 3, Aug. 1977, p. 353-358. In Russian.

Astronomy and Astrophysics

Astronomy

10

Gravitational Collapse, Metallic Stars, Stellar Rotation, Centrifugal Force, Hydrostatics, Nebulae, Neutrinos, Neutron Stars, Stellar Models, Stellar Radiation, Stellar Structure

Scientific paper

The spherically symmetric gravitational collapse of a two-solar-mass iron-oxygen stellar core is calculated. The initial configuration is a polytrope with an index n = 3, and rotation is taken into account in a one-dimensional approximation where the centrifugal force is averaged over a solid angle. The results show that no significant shell ejection occurs and that rotation may produce a substantial decrease in the neutrino luminosity of the collapsing star.

Affiliated with

Also associated with

No associations

Rating

Gravitational collapse of rotating iron-oxygen stars 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 Gravitational collapse of rotating iron-oxygen stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Gravitational collapse of rotating iron-oxygen stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1881304