Please use this identifier to cite or link to this item: http://hdl.handle.net/2445/99393
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dc.contributor.authorMigliari, Simone-
dc.contributor.authorFender, R. P.-
dc.contributor.authorRupen, M.-
dc.contributor.authorWachter, S.-
dc.contributor.authorJonker, P. G.-
dc.contributor.authorHoman, J.-
dc.contributor.authorVan der Klis, M.-
dc.date.accessioned2016-06-09T14:02:13Z-
dc.date.available2016-06-09T14:02:13Z-
dc.date.issued2004-06-
dc.identifier.issn0035-8711-
dc.identifier.urihttp://hdl.handle.net/2445/99393-
dc.description.abstractWe present the analysis of simultaneous X-ray (RXTE) and radio (VLA) observations of two atoll-type neutron star X-ray binaries: 4U 1820 - 30 and Ser X-1. Both sources were steadily in the soft (`banana') X-ray state during the observations. We have detected the radio counterpart of 4U 1820 - 30 at 4.86 and 8.46 GHz at a flux density of ~0.1 mJy. This radio source is positionally coincident with the radio pulsar PSR 1820 - 30A. However, the radio emission of the pulsar falls rapidly with frequency (~ν-3), and we argue that the radio emission of the X-ray binary is dominant above ~2 GHz. Supporting this interpretation, comparison with previous observations reveals variability at the higher radio frequencies that is likely to be due to the X-ray binary. We have detected for the first time the radio counterpart of Ser X-1 at 8.46 GHz, also at a flux density of ~0.1 mJy. The position of the radio counterpart has allowed us to identify its optical counterpart unambiguously. We briefly discuss similarities and differences between the disc-jet coupling in neutron star and black hole X-ray binaries. In particular, we draw attention to the fact that, contrary to other states, neutron star X-ray binaries seem to be more radio-loud than persistent black hole candidates when the emission is `quenched' in the soft state.-
dc.format.extent7 p.-
dc.format.mimetypeapplication/pdf-
dc.language.isoeng-
dc.publisherRoyal Astronomical Society-
dc.relation.isformatofReproducció del document publicat a: http://dx.doi.org/10.1111/j.1365-2966.2004.07768.x-
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society, 2004, vol. 351, num. 1, p. 186-192-
dc.relation.urihttp://dx.doi.org/10.1111/j.1365-2966.2004.07768.x-
dc.rights(c) Migliari, Simone et al., 2004-
dc.subject.classificationEstels binaris de raigs X-
dc.subject.classificationEstels de neutrons-
dc.subject.classificationAstronomia de raigs X-
dc.subject.otherX-ray binaries-
dc.subject.otherNeutron stars-
dc.subject.otherX-ray astronomy-
dc.titleRadio detections of the neutron star X-ray binaries 4U 1820 - 30 and Ser X-1 in soft X-ray states-
dc.typeinfo:eu-repo/semantics/article-
dc.typeinfo:eu-repo/semantics/publishedVersion-
dc.identifier.idgrec634035-
dc.date.updated2016-06-09T14:02:18Z-
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess-
Appears in Collections:Articles publicats en revistes (Física Quàntica i Astrofísica)

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