A comparison of radio emission from neutron star and black hole X-ray binaries

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dc.creatorFender, R. P.
dc.date1999-11-03
dc.date.accessioned2026-07-07T02:34:12Z
dc.date.available2026-07-07T02:34:12Z
dc.descriptionI compare the properties of radio emission from neutron star and black hole X-ray binaries. In both transient and persistent systems the ratio of X-ray : radio fluxes is comparable for (low field) neutron stars and black holes. It appears that, broadly speaking, the disc : jet coupling is independent of the nature of the accretor, (except for X-ray pulsars where the strong magnetic field prevents formation of an inner accretion disc and jet).
dc.descriptionTo be published in Proc. NATO advanced study institute `The Neutron Star - Black Hole connection'
dc.identifierhttps://arxiv.org/abs/astro-ph/9911032
dc.identifierhttp://arxiv.org/abs/astro-ph/9911032
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/15153
dc.subjectAstrophysics
dc.titleA comparison of radio emission from neutron star and black hole X-ray binaries
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