Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1620
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dc.contributor.authorMitra, D.-
dc.contributor.authorRamachandran, R.-
dc.date.accessioned2006-12-27T06:42:06Z-
dc.date.available2006-12-27T06:42:06Z-
dc.date.issued2001-05-
dc.identifier.citationAstronomy and Astrophysics, 2001, Vol.370, p586-590en
dc.identifier.issn0004-6361-
dc.identifier.urihttp://hdl.handle.net/2289/1620-
dc.description.abstractWe have measured the scatter broadening of pulsars in the direction of the Gum nebula. For the first time, our observations show clear variations of scattering properties across the Gum nebula. The IRAS-Vela shell is shown to be a high scattering region. Our revised estimations of distances to these pulsars are consistently less by a factor of 2-3, which has very important consequences for the deduced values of radio luminosity and transverse velocity of pulsars.en
dc.format.extent146682 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherEDP Sciencesen
dc.relation.urihttp://dx.doi.org/10.1051/0004-6361:20010274en
dc.rights(2001) by the European Southern Observatory.en
dc.subjectISM: GUM NEBULAen
dc.subjectSTARS: PULSARS: GENERALen
dc.titleScatter broadening of pulsars in the direction of the Gum nebulaen
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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