Please use this identifier to cite or link to this item: http://hdl.handle.net/2445/170933
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dc.contributor.authorSolà Peracaula, Joan-
dc.contributor.authorParedes i Poy, Josep Maria-
dc.contributor.authorTaylor, A.R.-
dc.contributor.authorDougherty, S.M.-
dc.contributor.authorScott, W.K.-
dc.date.accessioned2020-09-29T10:37:36Z-
dc.date.available2020-09-29T10:37:36Z-
dc.date.issued2001-01-01-
dc.identifier.issn0004-640X-
dc.identifier.urihttp://hdl.handle.net/2445/170933-
dc.description.abstractThe HALCA spacecraft in combination with a large array of ground radio telescopes has been used to obtain multi-epoch images of a radio outburst of the radio emitting, X-ray binary star LSI+61o303. Preliminary results from two 6-hour segments separated by 28.6 hours are presented. The images reveal an apparently stationary pattern of symmetric emission extending about 2 mas on either side of a central source. The extended emission is reminiscent of the precessing radio jets seen in SS433. The central source is observed to expand at a rate of 0.2 mas/day. At the distance of LSI+61o303, this corresponds to about700 km s^-1.-
dc.format.extent2 p.-
dc.format.mimetypeapplication/pdf-
dc.language.isoeng-
dc.publisherSpringer Science + Business Media-
dc.relation.isformatofVersió postprint del document publicat a: https://doi.org/10.1023/A:1011602219827-
dc.relation.ispartofAstrophysics and Space Science, 2001, vol. 276, p. 123-124-
dc.relation.urihttps://doi.org/10.1023/A:1011602219827-
dc.rights(c) Springer Science + Business Media, 2001-
dc.sourceArticles publicats en revistes (Física Quàntica i Astrofísica)-
dc.subject.classificationCosmologia-
dc.subject.otherCosmology-
dc.titleVSOP observations of the X-ray binary LSI+61303-
dc.typeinfo:eu-repo/semantics/article-
dc.typeinfo:eu-repo/semantics/acceptedVersion-
dc.identifier.idgrec186506-
dc.date.updated2020-09-29T10:37:36Z-
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess-
Appears in Collections:Articles publicats en revistes (Física Quàntica i Astrofísica)

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