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20012003
most citedA deep Chandra observation of the Perseus cluster: shocks and ripples

620 citations · 1.5k across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph2003★ 620 cited

A deep Chandra observation of the Perseus cluster: shocks and ripples

A. C. Fabian, J. S. Sanders, S. W. Allen +5

We present preliminary results from a deep observation lasting almost 200 ks, of the centre of the Perseus cluster of galaxies around NGC 1275. The X-ray surface brightness of the…

astro-ph2002★ 283 cited

Cosmological constraints from the X-ray gas mass fraction in relaxed lensing clusters observed with Chandra

S. W. Allen, R. W. Schmidt, A. C. Fabian

We present precise measurements of the X-ray gas mass fraction for a sample of luminous, relatively relaxed clusters of galaxies observed with the Chandra Observatory, for which in…

astro-ph2002★ 114 cited

Conduction and cooling flows

L. M. Voigt, R. W. Schmidt, A. C. Fabian +2

Chandra and XMM-Newton observations have confirmed the presence of large temperature gradients within the cores of many relaxed clusters of galaxies. Here we investigate whether th…

astro-ph2001★ 116 cited

Chandra observations of RXJ1347.5-1145: the distribution of mass in the most X-ray luminous galaxy cluster known

S. W. Allen, R. W. Schmidt, A. C. Fabian

We present Chandra observations of RXJ1347.5-1145, the most X-ray luminous cluster of galaxies known. We report the discovery of a region of relatively hot, bright X-ray emission,…

astro-ph2001★ 282 cited

The X-ray virial relations for relaxed lensing clusters observed with Chandra

S. W. Allen, R. W. Schmidt, A. C. Fabian

We examine the relations linking mass, X-ray temperature and bolometric luminosity for a sample of luminous, relatively relaxed clusters of galaxies observed with the Chandra Obser…

astro-ph2001★ 110 cited

Chandra observations of the galaxy cluster Abell 1835

R. W. Schmidt, S. W. Allen, A. C. Fabian

We present the analysis of 30 ksec of Chandra observations of the galaxy cluster Abell 1835. Overall, the X-ray image shows a relaxed morphology, although we detect substructure in…