activity
19972004
most citedChandra temperature profiles for a sample of nearby relaxed galaxy clusters

527 citations · 530 across the 3 of their papers we have counts for

collaborators

7 papers

astro-ph2004527 cited

Chandra temperature profiles for a sample of nearby relaxed galaxy clusters

A. Vikhlinin, M. Markevitch, S. S. Murray +3

We present Chandra gas temperature profiles at large radii for a sample of 13 nearby, relaxed galaxy clusters and groups, which includes A133, A262, A383, A478, A907, A1413, A1795,…

astro-ph20041 cited

Cen A and its interaction with the x-ray emitting interstellar medium

D. M. Worrall, R. P. Kraft, M. Birkinshaw +4

As the closest radio galaxy, Centaurus A is a powerful laboratory for the X-ray study of radio-emitting structures and their interactions with the hot interstellar medium (ISM). Th…

astro-ph20032 cited

A High Angular Resolution View of Hot Gas in Clusters, Groups, and Galaxies

W. Forman, E. Churazov, L. David +6

We discuss two themes from Chandra and XMM-Newton observations of galaxies, groups, and clusters. First, we review observational aspects of cluster formation and evolution as matte…

astro-ph2002

Two Years of the X-ray Sky in M31

A. K. H. Kong, M. R. Garcia, F. A. Primini +2

We have been monitoring M31 with HRC and ACIS onboard \chandra regularly in the past two years. By combining eight \chandra ACIS-I observations taken between 1999 to 2001, we have…

astro-ph2001

Exploring the Early Universe with XMM-Newton

I. Lehmann, G. Hasinger, S. S. Murray +1

The question of the X-ray background has been largely settled over the last 10 years using the ROSAT satellite. About 70-80 % of the soft X-ray background was resolved into discret…

astro-ph2000

Chandra Observations of M31 and their Implications for its ISM

F. Primini, M. Garcia, S. Murray +3

We have been regularly observing the bulge and inner disk of M31 for nearly 1 year, using both the HRC-I and ACIS-I instruments on the Chandra X-Ray Observatory. We present results…