More about collapse of a radiating star

Details More about collapse of a radiating star More about collapse of a radiating star

May 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986mnras.220..405d&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 220, May 15, 1986, p. 405-412.

Astronomy and Astrophysics

Astronomy

20

Gravitational Collapse, Neutron Stars, Stellar Models, Stellar Radiation, White Dwarf Stars, Gamma Rays, Pulsed Radiation, X Rays

Scientific paper

The de Oliveira et al. (1985) model is used to predict the properties of the strong radiation pulse in the optical, X-ray, and gamma-ray domains that results from the collapse of neutron stars and white dwarfs in rapid mass-loss phases. The calculations indicate that the distinct temporal behavior of the pulses in different spectral regions permit the observational discrimination of various collapsing star models. Attention is given to the unresolved character of the gamma-ray burst sources of Klebesadel et al. (1973).

Affiliated with

Also associated with

No associations

Rating

More about collapse of a radiating star 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 More about collapse of a radiating star, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and More about collapse of a radiating star will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1774972