Enigmatic sub-luminous accreting neutron stars in our Galaxy
| Authors | |
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| Publication date | 2008 |
| Host editors |
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| Book title | A Population Explosion: The Nature & Evolution of X-ray Binaries in Diverse Environments |
| Book subtitle | St. Pete Beach, Florida, 28 October-2 November 2007 |
| ISBN |
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| Series | AIP Conference Proceedings |
| Event | A Population Explosion: The Nature & Evolution of X-ray Binaries in Diverse Environments, St. Pete Beach, FL, USA |
| Pages (from-to) | 382-386 |
| Publisher | Melville, NY: American Institute of Physics |
| Organisations |
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| Abstract | During the last few years a class of enigmatic sub‐luminous accreting neutron stars has been found in our Galaxy. They have peak X‐ray luminosities (2–10 keV) of a few times 1034 erg s−1 to a few times 1035 erg s−1, and both persistent and transient sources have been found. I present a short overview of our knowledge of these systems and what we can learn from them. |
| Document type | Conference contribution |
| Language | English |
| Published at | https://doi.org/10.1063/1.2945081 |
| Downloads |
301974.pdf
(Accepted author manuscript)
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