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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1503
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dc.contributor.authorVivekanand, M.-
dc.contributor.authorMohanty, D.K.-
dc.contributor.authorSalter, C.J.-
dc.date.accessioned2006-11-04T11:36:24Z-
dc.date.available2006-11-04T11:36:24Z-
dc.date.issued1983-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, 1983, Vol.204, p81-en
dc.identifier.issn0035-8711-
dc.identifier.urihttp://hdl.handle.net/2289/1503-
dc.descriptionOpen Accessen
dc.description.abstractImproved declinations have been measured for 40 weak pulsars with the Ooty Radio Telescope, together with flux densities at 327 MHz. For 32 of the pulsars, improved periods have been derived. It is demonstrated that PSR1922 + 20 is highly unlikely to be associated with the radio continuum source 4C 20.48.en
dc.format.extent8338 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherBlackwell Publishing for the Royal Astronomical Societyen
dc.relation.urihttp://adsabs.harvard.edu/cgi-bin/bib_query?1983MNRAS.204P..81Ven
dc.relation.urihttp://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983MNRAS.204P..81V&link_type=ARTICLE&db_key=ASTen
dc.rights(1983) Royal Astronomical Societyen
dc.subjectASTROMETRY,en
dc.subjectDECLINATION,en
dc.subjectPULSARS,en
dc.subjectPERIODIC VARIATIONS,en
dc.subjectRADIANT FLUX DENSITY,en
dc.subjectRADIO SOURCES (ASTRONOMY)en
dc.titleImproved parameters for 40 pulsarsen
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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