Neutron Stars and Black Holes in Globular Clusters

Details Neutron Stars and Black Holes in Globular Clusters Neutron Stars and Black Holes in Globular Clusters

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998tx19.confe.219r&link_type=abstract

Abstracts of the 19th Texas Symposium on Relativistic Astrophysics and Cosmology, held in Paris, France, Dec. 14-18, 1998. Eds.:

Astronomy and Astrophysics

Astrophysics

Scientific paper

If neutron stars can be turned into low-mass (1.5-3 M_odot) black holes by accretion of gas following a collision with another star, or because of fall-back of material after the supernova explosion, there should be a significant population of such low-mass black holes in globular clusters. The consequences of such a population will be discussed and compared with observations of X-ray sources and radio pulsars in clusters.

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