Collapse of a radiating star revisited

Details Collapse of a radiating star revisited Collapse of a radiating star revisited

Apr 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988mnras.231.1011d&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 231, April 15, 1988, p. 1011-1018.

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18

Gravitational Collapse, Stellar Luminosity, Stellar Radiation, Black Holes (Astronomy), Computational Astrophysics, Red Shift, Time Dependence

Scientific paper

Some further results are obtained concerning the solution by Oliveira et al. (1986) to the model of a collapsing star consisting of a spherically symmetric nonadiabatic fluid which produces a pure radiation field. The collapsing fluid is isotropic with dissipation under a radial heat flow. The model is studied here without imposing any particular initial static configuration. It is shown that some of the model properties depend only upon its initial mass and the initial radius of the fluid distribution.

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