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Discovery of a High-Energy Gamma-Ray-Emitting Persistent Microquasar

Open access
Paredes, Josep M., Martı́, Josep, Ribó, Marc, Massi, Maria·2000·Science

Abstract

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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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.