Diffuse radio emission from the Coma cluster of galaxies at decameter  wavelengths

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1054

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DC Field	Value	Language
dc.contributor.author	Sastry, Ch.V.	-
dc.contributor.author	Shevgaonkar, R.K.	-
dc.date.accessioned	2006-01-03T04:49:35Z	-
dc.date.available	2006-01-03T04:49:35Z	-
dc.date.issued	1983	-
dc.identifier.citation	Journal of Astrophysics and Astronomy, 1983, Vol. 4, p47-51.	en
dc.identifier.issn	0250-6335	-
dc.identifier.uri	http://hdl.handle.net/2289/1054	-
dc.description.abstract	A 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.extent	270707 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Indian Academy of Sciences, Bangalore, India.	en
dc.rights	Indian Academy of Sciences, Bangalore, India.	en
dc.subject	Cluster of galaxies	en
dc.subject	Intracluster medium	en
dc.subject	Radio spectra	en
dc.title	Diffuse radio emission from the Coma cluster of galaxies at decameter wavelengths	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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