Two new bright X-ray sources in globular clusters, and many less luminous ones in globular clusters and in old open clusters, have been discovered with ROSAT. Accurate positions obtained with ROSAT help identification with optical objects, which however is still very incomplete in globular clusters. One dim globular cluster source has been identified with a recycled radio pulsar; several others may be cataclysmic variables. The four brightest X-ray sources identified in the old open cluster M67 are puzzling, as we do not understand why they emit X-rays. In comparison with the two old open clusters studied so far, globular clusters are remarkably underluminous in X-rays
Evolution of the X-ray cluster luminosity function (XLF) has been investigated through X-ray observa...
A ROSAT x-ray survey, with complimentary optical photometry, of the open cluster NGC 6475 has enable...
M67 is an old open star cluster with an estimated age of ~4 billion years. It is one of the best st...
I analyze 101 observations from the ROSAT archive to search for X-ray sources in or near 55 globular...
This grant supported our analysis of ROSAT x-ray data on globular clusters. Although the grant title...
The twelve bright (Lx>10(36) erg/s) X-ray sources in the globular clusters have lower luminosities t...
I analyze 101 observations from the ROSAT archive to search for X-ray sources in or near 55 globula...
A ROSAT HRI X-ray image was obtained of the open globular cluster NGC 288, which is located near the...
The X-ray sky is host to a variety of objects with very distinct properties and underlying physics. ...
In the construction of an X-ray-selected sample of galaxy clusters for cosmological studies, we have...
The goal of these ROSAT PSPC pointed observations was to understand the nature of X-ray emission ass...
We present an X-ray analysis of a 4 Gyr old open cluster, M67, using archival XMM–Newton data. The a...
Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 2003.Includes bibliographi...
We report on 40 kiloseconds of ROSAT HRI observations of the globular cluster M92 (NGC 6341) and 20 ...
We present the results of a joint ROSAT High Resolution Imager (HRI) and optical investigation of th...
Evolution of the X-ray cluster luminosity function (XLF) has been investigated through X-ray observa...
A ROSAT x-ray survey, with complimentary optical photometry, of the open cluster NGC 6475 has enable...
M67 is an old open star cluster with an estimated age of ~4 billion years. It is one of the best st...
I analyze 101 observations from the ROSAT archive to search for X-ray sources in or near 55 globular...
This grant supported our analysis of ROSAT x-ray data on globular clusters. Although the grant title...
The twelve bright (Lx>10(36) erg/s) X-ray sources in the globular clusters have lower luminosities t...
I analyze 101 observations from the ROSAT archive to search for X-ray sources in or near 55 globula...
A ROSAT HRI X-ray image was obtained of the open globular cluster NGC 288, which is located near the...
The X-ray sky is host to a variety of objects with very distinct properties and underlying physics. ...
In the construction of an X-ray-selected sample of galaxy clusters for cosmological studies, we have...
The goal of these ROSAT PSPC pointed observations was to understand the nature of X-ray emission ass...
We present an X-ray analysis of a 4 Gyr old open cluster, M67, using archival XMM–Newton data. The a...
Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 2003.Includes bibliographi...
We report on 40 kiloseconds of ROSAT HRI observations of the globular cluster M92 (NGC 6341) and 20 ...
We present the results of a joint ROSAT High Resolution Imager (HRI) and optical investigation of th...
Evolution of the X-ray cluster luminosity function (XLF) has been investigated through X-ray observa...
A ROSAT x-ray survey, with complimentary optical photometry, of the open cluster NGC 6475 has enable...
M67 is an old open star cluster with an estimated age of ~4 billion years. It is one of the best st...