Using SKA to observe relativistic jets from X-ray binary systems

Authors
Publication date 2004
Journal New Astronomy Reviews
Volume | Issue number 48
Pages (from-to) 1399-1412
Organisations
  • Faculty of Science (FNWI) - Anton Pannekoek Institute for Astronomy (API)
Abstract I briefly outline our current observational understanding of the relativistic jets observed from X-ray binary systems, and how their study may shed light on analogous phenomena in active galactic nuclei and gamma ray bursts. How SKA may impact on this field is sketched, including the routine tracking of relativistic ejections to large distances from the binaries, detecting and monitoring the radio counterparts to `quiescent' black holes, and detecting the radio counterparts of the brightest X-ray binaries throughout the local group of galaxies.
Document type Article
Published at https://doi.org/10.1016/j.newar.2004.09.033
Published at http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004NewAR..48.1399F&db_key=AST&high=42079022cc15308
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