Final evolution of stars in the range 1,000 to 10,000 solar masses

Details Final evolution of stars in the range 1,000 to 10,000 solar masses Final evolution of stars in the range 1,000 to 10,000 solar masses

Aug 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977ap%26ss..50..125w&link_type=abstract

Astrophysics and Space Science, vol. 50, no. 1, Aug. 1977, p. 125-131. NSF-supported research.

Astronomy and Astrophysics

Astrophysics

13

Gravitational Collapse, Stellar Evolution, Stellar Mass, Astrodynamics, Astronomical Models, Cores, Cosmology, Globular Clusters, Nuclear Fusion, Oxygen, X Ray Sources

Scientific paper

The final dynamical collapse of oxygen cores of 1,000 and 10,000 solar masses which undergo the pair formation instability is computed. These cores are found to suffer complete collapse, presumably to form black holes, in contrast to cores approximately 100 solar masses which have previously been found to explode completely, leaving no remnant. These calculations represent a first attempt to ascertain the outcome over several decades of the evolution of mass amounts previously unstudied. The outcome may have some relevance to models of X-ray sources in globular clusters.

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