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Discovery of a High-Energy Gamma-Ray-Emitting Persistent Microquasar
Open accessAbstract
Microquasars are stellar x-ray binaries that behave as a scaled-down version of extragalactic quasars. The star LS 5039 is a new microquasar system with apparent persistent ejection of relativistic plasma at a 3-kiloparsec distance from the sun. It may also be associated with a γ-ray source discovered by the Energetic Gamma Ray Experiment Telescope (EGRET) on board the COMPTON–Gamma Ray Observatory satellite. Before the discovery of LS 5039, merely a handful of microquasars had been identified in the Galaxy, and none of them was detected in high-energy γ-rays.
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Cited by
THE LARGE AREA TELESCOPE ON THE FERMI GAMMA-RAY SPACE TELESCOPE MISSION
Atwood, W. B., Abdo, A. A., Ackermann, M., Althouse, W., Anderson, B., Axelsson, M., Baldini, L., Ballet, J., Band, D. L., Barbiellini, G., et al. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/697/2/1071 · Cited by 4,198
Gamma-ray binaries: pulsars in disguise?
Dubus, G. (2006) · Astronomy & Astrophysics · doi:10.1051/0004-6361:20054779 · Cited by 270
Metadata
- Authors
- Paredes, J. M., Martı́, J., Ribó, M., & Massi, M.
- Venue
- Science
- Published
- 2000-06-30
- Volume
- 288
- Issue
- 5475
- Pages
- 2340-2342
- ISSN
- 0036-8075 (ISSN-L)
- 1095-9203
- OpenAlex
- W2124799392
- Cited by
- 324
- References
- 0
- FWCI
- 17.54
- Type
- journal article
- Language
- en
- Open access
- green
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- CoChat. (2026). Citation check: Discovery of a High-Energy Gamma-Ray-Emitting Persistent Microquasar. https://app.cochat.ai/papers/10.1126/science.288.5475.2340
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- Paredes, J. M., Martı́, J., Ribó, M., & Massi, M. (2000). Discovery of a High-Energy Gamma-Ray-Emitting Persistent Microquasar. Science. https://doi.org/10.1126/science.288.5475.2340
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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.