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

2000/06/30 by J. M. Paredes, J. Martı́, J. Marti +3 · 12 citations
Physics and Astronomy · #Astrophysics #Astrophysics and Cosmic Phenomena #Energy (signal processing) #Gamma ray #Gamma-ray bursts and supernovae #Physics #Radio Astronomy Observations and Technology #astro-ph

paper · pdf · doi:10.1126/science.288.5475.2340

published as Science288:2340,2000 · 13 pages, 3 figures, LaTeX, uses aaspp4.sty. Published in Science, 2000 June 30. Related papers may be found at http://www.am.ub.es/~josep/papers/index.html

openalex publication_date 2000/06/30 · arxiv created 2001/02/13 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

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 gamma-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 gamma-rays.

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