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Elemental Abundances of Nearby Galaxies through High Signal-to-Noise XMM-Newton Observations of ULXs
Lisa M. Winter, Richard F. Mushotzky, Christopher S. Reynolds
(abridged) In this paper, we examined XMM Newton EPIC spectra of 14 ultra-luminous X-ray sources (ULXs)in addition to the XMM RGS spectra of two sources (Holmberg II X-1 and Holmbe…
Constraining Black Hole Spin Via X-ray Spectroscopy
Laura W. Brenneman, Christopher S. Reynolds
We present an analysis of the observed broad iron line feature and putative warm absorber in the long 2001 XMM-Newton observation of the Seyfert-1.2 galaxy MCG-6-30-15. The new "ke…
Trapping of magnetic flux by the plunge region of a black hole accretion disk
Christopher S. Reynolds, David Garofalo, Mitchell C. Begelman
The existence of the radius of marginal stability means that accretion flows around black holes invariably undergo a transition from a MHD turbulent disk-like flow to an inward plu…
The influence of radio-galaxy activity on X-ray absorption lines from the intracluster medium
Franziska Koeckert, Christopher S. Reynolds
We present an investigation of the X-ray absorption features predicted by hydrodynamic simulations of radio galaxies interacting with the intracluster medium (ICM) of their host ga…