Evidence for Intermediate Mass Black Holes in Ultra-Luminous X-ray Sources

Details Evidence for Intermediate Mass Black Holes in Ultra-Luminous X-ray Sources Evidence for Intermediate Mass Black Holes in Ultra-Luminous X-ray Sources

Sep 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..352..121m&link_type=abstract

New Horizons in Astronomy: Frank N. Bash Symposium ASP Conference Series, Vol. 352, Proceedings of the Conference Held 16-18 Oct

Astronomy and Astrophysics

Astronomy

Scientific paper

It is becoming clear that intermediate-mass black holes --- black holes with masses in the 100--10,000 M&sun; range --- may have played an important role in early galactic evolution, and may currently be playing an important role in stellar cluster evolution. Here, I briefly highlight emerging evidence for intermediate mass black holes, in a subset of the most luminous non-nuclear X-ray point sources in nearby normal galaxies.

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