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19952023
most citedThe Quiescent Intracluster Medium in the Core of the Perseus Cluster

500 citations · 2.7k across the 43 of their papers we have counts for

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Showing 2003 · astro-phShow all

6 papers · 2 filters

astro-ph2003

XMM Observations of an IXO in NGC 2276

David S. Davis, Richard F. Mushotzky

We present the results from a ~53 ksec XMM observation of NGC 2276. This galaxy has an unusual optical morphology with the disk of this spiral appearing to be truncated along the w…

astro-ph2003

Probable intermediate mass black holes in NGC4559: XMM-Newton spectral and timing constraints

Mark Cropper, Roberto Soria, Richard F. Mushotzky +3

We have examined X-ray and optical observations of two ultra-luminous X-ray sources, X7 and X10 in NGC4559, using XMM-Newton, Chandra and HST. The UV/X-ray luminosity of X7 exceeds…

astro-ph2003

The Changing AGN Population

A. T. Steffen, A. J. Barger, L. L. Cowie +2

We investigate how the fraction of broad-line sources in the AGN population changes with X-ray luminosity and redshift. We first construct the rest-frame hard-energy (2-8 keV) X-ra…

astro-ph2003

Chandra Observations of Point Sources in Abell 2255

D. S. Davis, N. A. Miller, R. F. Mushotzky

In our search for ``hidden'' AGN we present results from a Chandra observation of the nearby cluster Abell 2255. Eight cluster galaxies are associated with point-like X-ray emissio…

astro-ph2003

Discovery of X-ray QPOs from an Ultra-luminous X-ray Source in M82: Evidence Against Beaming

Tod E. Strohmayer, Richard F. Mushotzky

We report the discovery with the EPIC CCD cameras onboard XMM-Newton of a 54 mHz quasiperiodic oscillation (QPO) in the > 2 keV X-ray flux from an ultraluminous X-ray source (ULX)…

astro-ph2003

Groups and the Entropy Floor- XMM-Newton Observations of Two Groups

R. Mushotzky, E. Figueroa-Feliciano, M. Loewenstein +1

Using XMM-Newton spatially resolved X-ray imaging spectroscopy we obtain the temperature, density, entropy, gas mass, and total mass profiles for two groups of galaxies out to ~0.3…