Electromagnetic and Gravitational-Wave Signatures of the Earliet Supermassive Black Holes

Details Electromagnetic and Gravitational-Wave Signatures of the Earliet Supermassive Black Holes Electromagnetic and Gravitational-Wave Signatures of the Earliet Supermassive Black Holes

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003head....7.2801l&link_type=abstract

American Astronomical Society, HEAD meeting #7, #28.01; Bulletin of the American Astronomical Society, Vol. 35, p.647

Astronomy and Astrophysics

Astronomy

Scientific paper

Black holes weighing more than a billion solar masses are known to exist
at a redshift of 6, only a billion years after the big bang. I will
describe simple theoretical models for their formation and growth. These
models predict gravitational wave and X-ray signatures that will be
testable with future missions, such as LISA, Con-X and EXIST.

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