activity
19972005
most citedThe temperature structure in the core of Sersic 159-03

35 citations · 38 across the 4 of their papers we have counts for

collaborators

11 papers

astro-ph200535 cited

The temperature structure in the core of Sersic 159-03

J. de Plaa, J. S. Kaastra, M. Mendez +6

We present results from a new 120 ks XMM-Newton observation of the cluster of galaxies Sersic 159-03. In this paper we focus on the high-resolution X-ray spectra obtained with the…

astro-ph20031 cited

High Resolution X-ray Spectroscopic Constraints on Cooling-Flow Models

John R. Peterson, Steven M. Kahn, Frits B. S. Paerels +5

We present XMM-Newton Reflection Grating Spectrometer observations of X-ray clusters and groups of galaxies. We demonstrate the failure of the standard cooling-flow model to descri…

astro-ph2002

XMM-Newton Measurements of the Elemental Abundances in the Intracluster Medium

T. Tamura, J. S. Kaastra, J. A. M. Bleeker +1

Based on XMM-Newton observations of a sample of galaxy clusters, we have measured the elemental abundances (mainly O, Si, S, and Fe) and their spatial distributions in the intraclu…

astro-ph20022 cited

The Milky Way - Pulsars and Isolated Neutron Stars

W. Becker, G. G. Pavlov

CONTENTS The Milky Way -- Pulsars and Isolated Neutron Stars / Introduction: Historical Overview / Physics and Astrophysics of Isolated Neutron Stars / Rotation-powered Pulsars: Th…

astro-ph2002

Non-thermal bremsstrahlung as the dominant hard X-ray continuum emission from the supernova remnant MSH14-63 (RCW 86)

Jacco Vink, Johan Bleeker, Jelle Kaastra +3

We present an analysis of the X-ray emission of the supernova remnant MSH14-63, which was partially covered by four observations with XMM-Newton. The detection of Fe K emission at…

astro-ph2002

A synoptic spectral study of Cassiopeia-A based on XMM-Newton and BeppoSax observations

Johan Bleeker, Jacco Vink, Kurt van der Heyden +3

In this paper we present recent image and spectral data of Cas-A obtained with XMM-Newton and BeppoSAX. Analysis of the hard X-ray continuum does not support an interpretation of t…