General Relativity studies through X-ray spectroscopy of the Fe (and others) K α fluorescent lines

Details General Relativity studies through X-ray spectroscopy of the Fe (and others) K α fluorescent lines General Relativity studies through X-ray spectroscopy of the Fe (and others) K α fluorescent lines

Apr 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ap%26ss.320..129g&link_type=abstract

Astrophysics and Space Science, Volume 320, Issue 1-3, pp. 129-134

Astronomy and Astrophysics

Astrophysics

X-Ray: Galaxies, Galaxies: Quasars, Emission Lines, Galaxies: Active, Lines: Profiles, Lines: Formation, Accretion Disks

Scientific paper

I briefly review in this paper the main observational properties of relativistically broadened X-ray spectral lines in Galactic Black Holes and Active Galactic Nuclei, and the (scanty) estimates of their frequency in the corresponding parent populations. The available measurements allow us to derive some constraints on the black hole spin and mass, and on the accretion disk geometry and illumination.

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