Collapse of iron stellar cores

Details Collapse of iron stellar cores Collapse of iron stellar cores

Dec 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...263..366b&link_type=abstract

Astrophysical Journal, Part 1, vol. 263, Dec. 1, 1982, p. 366-376.

Astronomy and Astrophysics

Astronomy

71

Gravitational Collapse, Metallic Stars, Stellar Cores, Stellar Evolution, Stellar Models, Black Holes (Astronomy), Electron Capture, Equations Of State, Iron, Nuclear Interactions, Shock Wave Propagation

Scientific paper

The collapse of the iron core of evolved 10, 15, and 20 solar mass stars has been calculated using a spherically symmetric numerical model. No bounce occurs and no matter is ejected. Sensitivity to some less well-established details, and to zoning, has been examined and the overall qualitative results are unchanged. A black hole is the presumed outcome of the model.

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