Scattering model for X-ray bursts - Massive black holes in globular clusters

Details Scattering model for X-ray bursts - Massive black holes in globular clusters Scattering model for X-ray bursts - Massive black holes in globular clusters

May 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...205l.131g&link_type=abstract

Astrophysical Journal, vol. 205, May 1, 1976, pt. 2, p. L131-L133.

Astronomy and Astrophysics

Astronomy

54

Astronomical Models, Black Holes (Astronomy), Compton Effect, Globular Clusters, X Ray Scattering, X Ray Sources, Decay Rates, Energy Spectra, Gravitational Collapse, Time Constant

Scientific paper

A model for the X-ray bursts discovered from 3U 1820-30 (NGC 6624) is presented. The temporal and spectral variations observed in the bursts are interpreted as Compton scattering of a primary pulse in a hot cloud surrounding the X-ray source. The cloud parameters derived imply the presence of a collapsed core in the globular cluster source with a mass greater than several hundred solar masses.

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