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 |