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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1559
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dc.contributor.authorDeshpande, A.A.-
dc.contributor.authorMcCulloch, P.M.-
dc.contributor.authorRadhakrishnan, V.-
dc.contributor.authorAnantharamaiah, K.R.-
dc.date.accessioned2006-12-05T11:14:48Z-
dc.date.available2006-12-05T11:14:48Z-
dc.date.issued1992-09-01-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, 1992, Vol.258, p19-21en
dc.identifier.issn0035-8711-
dc.identifier.urihttp://hdl.handle.net/2289/1559-
dc.descriptionOpen Accessen
dc.description.abstractIf small-scale structure is present in H I clouds, then H I absorption profiles toward pulsars with large proper motions should show changes on a time-scale of a few years. We have compared absorption measurements, made with an interval of about four years, toward two pulsars and find a marginal difference in one of them. If confirmed, this could imply structures on the scale of about 1000 AU in H I clouds.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?1992MNRAS.258P..19Den
dc.relation.urihttp://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992MNRAS.258P..19D&link_type=ARTICLE&db_key=ASTen
dc.rights(1992) Royal Astronomical Societyen
dc.subjectABSORPTION SPECTRA,en
dc.subjectH I REGIONS,en
dc.subjectINTERSTELLAR MATTER,en
dc.subjectPULSARS,en
dc.subjectEMISSION SPECTRA,en
dc.subjectRADIAL VELOCITYen
dc.titlePulsar observations and small-scale structure in interstellar H Ien
dc.typeArticleen
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