Detecting Isolated Accreting Black Holes

Details Detecting Isolated Accreting Black Holes Detecting Isolated Accreting Black Holes

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aas...198.8002a&link_type=abstract

American Astronomical Society, 198th AAS Meeting, #80.02; Bulletin of the American Astronomical Society, Vol. 33, p.908

Astronomy and Astrophysics

Astronomy

Scientific paper

The number of black holes present in the disk of the Milky Way galaxy
may be as large as 108 based on detections of long timescale
microlensing events. We argue that X-ray emission from about 10-1000
isolated accreting black holes should be detectable in the cores of
molecular clouds with future hard X-ray telescopes, such as EXIST.

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