Diffuse radio emission from the coma cluster of galaxies at decametre wavelengths

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4178

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DC Field	Value	Language
dc.contributor.author	Sastry, Ch. V	-
dc.contributor.author	Shevgaonkar, R. K	-
dc.date.accessioned	2008-12-29T11:55:28Z	-
dc.date.available	2008-12-29T11:55:28Z	-
dc.date.issued	1983-03	-
dc.identifier.citation	Journal of Astrophysics and Astronomy, Vol. 4, pp. 47 - 51	en
dc.identifier.issn	0250-6335	-
dc.identifier.uri	http://hdl.handle.net/2248/4178	-
dc.description	Open Access	-
dc.description.abstract	We have observed the region of the Coma cluster at 34.5 MHz with a resolution of 26 arcmin × 40 arcmin. A map of the diffuse halo (Coma C) is presented. The size of the halo is found to be 54 arcmin × 30 arcmin. The position angle is 50° ± 10° and the integrated flux is 60 ± 11 Jy. We have also found an extended source to the south of Coma A. The measured half-power widths of this source are 30 arcmin × 40 arcmin. The position angle is 135° and the integrated flux is ~ 15 Jy at 34.5 MHz. The spectral index in the frequency range 408 to 34.5 MHz is -1.0. It is suggested that this source also belongs to the Coma cluster.	en
dc.language.iso	en	en
dc.publisher	Indian Academy of Sciences	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1983JApA....4...47S	en
dc.relation.uri	http://dx.doi.org/10.1007/BF02714191	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 decametre wavelengths	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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