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29 March 2024
 
  » arxiv » astro-ph/0208086

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Pair Annihilation and Radio Emission from Nova Muscae
D.C. Hannikainen ; C.R. Kaiser ;
Date 5 Aug 2002
Subject astro-ph
Affiliation1,2) and C.R. Kaiser ( Observatory, University of Helsinki, Finland, Department of Physics & Astronomy, University of Southampton, UK
AbstractIn the hard X-ray spectra of some X-ray binaries line features around 500 keV are detected. We interpret these as arising from pair annihilation in relativistic outflows leading to a significant Doppler shift of the frequencies of the lines. We show that a small fraction of pairs escaping the annihilation region may give rise to the radio synchrotron emission observed in Nova Muscae 1991.
Source arXiv, astro-ph/0208086
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