Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1054
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dc.contributor.authorSastry, Ch.V.-
dc.contributor.authorShevgaonkar, R.K.-
dc.date.accessioned2006-01-03T04:49:35Z-
dc.date.available2006-01-03T04:49:35Z-
dc.date.issued1983-
dc.identifier.citationJournal of Astrophysics and Astronomy, 1983, Vol. 4, p47-51.en
dc.identifier.issn0250-6335-
dc.identifier.urihttp://hdl.handle.net/2289/1054-
dc.description.abstractA map of the diffuse halo, Coma C, is constructed on the basis of observations of the Coma Cluster at 34.5 MHz with a resolution of 26 X 40 arcmin. The position angle is 50 + or 10 deg, and the integrated flux is 60 + or - 11 Jy. An extended source is noted to the south of Coma A whose measured half-power widths are 30 X 40 arcmin. The position angle is 135 deg, and the integrated flux approximately 15 Jy at 34.5 MHz. It is suggested that this source also belongs to the Coma Cluster.en
dc.format.extent270707 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherIndian Academy of Sciences, Bangalore, India.en
dc.rightsIndian Academy of Sciences, Bangalore, India.en
dc.subjectCluster of galaxiesen
dc.subjectIntracluster mediumen
dc.subjectRadio spectraen
dc.titleDiffuse radio emission from the Coma cluster of galaxies at decameter wavelengthsen
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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