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19952003
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astro-ph20081 cited

2XMM J100451.6+411627: A cool core cluster at z=0.82

Matthias Hoeft, Georg Lamer, Jan Kohnert +1

- Aims: Gas cooling in the centre of massive galaxy clusters is believed to feed the most powerful active galactic nuclei in the Universe. How often clusters at high redshift show…

astro-ph2008

2XMM J083026+524133: The most X-ray luminous cluster at redshift 1

G. Lamer, M. Hoeft, J. Kohnert +2

In the distant universe X-ray luminous clusters of galaxies are rare objects. Large area surveys are therefore needed to probe the high luminosity end of the cluster population at…

astro-ph20077 cited

Proper motions of ROSAT discovered isolated neutron stars measured with Chandra: First X-ray measurement of the large proper motion of RX J1308.6+2127/RBS 1223

C. Motch, A. M. Pires, F. Haberl +2

The unprecedented spatial resolution of the Chandra observatory opens the possibility to detect with relatively high accuracy proper motions at X-ray wavelengths. We have conducted…

astro-ph2007

The ultra-compact binary candidate KUV 23182+1007 is a bright quasar

John Southworth, A. Schwope, B. T. Gaensicke +1

KUV 23182+1007 was identified as a blue object in the Kiso UV Survey in the 1980s. Classification-dispersion spectroscopy showed a featureless continuum except for a strong emissio…

astro-ph2003

X-rays from Cataclysmic Variables

Erik Kuulkers, Andrew Norton, Axel Schwope +1

Cataclysmic Variables are a distinct class of interacting binaries, transferring mass from a donor star to a degenerate accretor, a white dwarf. We here review X-ray observations o…

astro-ph2002

The XMM-Newton Bright Serendipitous Source Sample (XMM-Newton BSS)

R. Della Ceca, T. Maccacaro, A. Caccianiga +15

The XMM-Newton Survey Science Center is constructing a large (~1000 sources) and complete sample of bright serendipitous XMM-Newton sources at high galactic latitude, so as to allo…