Let's Challenge the Relativistic Radiation Hydrodynamics: 3 Observational Appearance of Black-Hole Winds

Details Let's Challenge the Relativistic Radiation Hydrodynamics: 3 Observational Appearance of Black-Hole Winds Let's Challenge the Relativistic Radiation Hydrodynamics: 3 Observational Appearance of Black-Hole Winds

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008asthe.101..576s&link_type=abstract

The Astronomical Herald (ISSN 0374-2466), Vol. 101, No. 10, p. 576 - 588 (2008)

Astronomy and Astrophysics

Astronomy

1

Scientific paper

Relativistic outflows are believed to blow off from quasars and active
galaxies, ultraluminous X-ray sources, microquasars, and gamma-ray
bursts. The authors examine the observational appearance of such an
outflow, a black-hole wind. As the flow velocity increases, an apparent
photosphere shrinks and an observed temperature and luminosity increase.

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