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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1593
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dc.contributor.authorMorris, D.-
dc.contributor.authorRadhakrishnan, V.-
dc.contributor.authorShukre, C.S.-
dc.date.accessioned2006-12-15T10:47:08Z-
dc.date.available2006-12-15T10:47:08Z-
dc.date.issued1978-08-
dc.identifier.citationAstronomy and Astrophysics, 1978, Vol.68, p289-293en
dc.identifier.issn0004-6361-
dc.identifier.urihttp://hdl.handle.net/2289/1593-
dc.description.abstractAn attempt is made to establish associations between pulsars and supernova remnants based not only on their distances, ages and position but also on pulsar radio polarization information. Of three pulsars investigated, a supernova remnant (G 193.3-1.5) is visible near one (PSR 0525 + 21) but the estimated ages of the remnant and the pulsar are discrepant. Possible ways of removing this discrepancy are discussed. Two further associations are proposed on the basis of position and distance estimates alone. They are PSR 0153 + 61 with G 132.4 + 2.2 (HB3) and PSR 1927 + 18 with G 53.9 + 0.3.en
dc.format.extent836385 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherSpringer-Verlagen
dc.relation.urihttp://adsabs.harvard.edu/cgi-bin/bib_query?1978A&A....68..289Men
dc.rights(1978) European Southern Observatory. Scanned images provided by the NASA ADS Data System.en
dc.subjectAstronomical modelsen
dc.subjectBinary starsen
dc.subjectPolarized Electromagnetic Radiationen
dc.subjectPulsarsen
dc.subjectStellar evolutionen
dc.subjectSupernova Remnantsen
dc.subjectInterstellar matteren
dc.subjectStellar luminosityen
dc.titleThree proposed pulsar/supernova remnant associations and their possible origin in close binary systemsen
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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