Observations of the supernova remnants HB 9 and IC 443 at 34.5 MHz

dc.contributor.author	Dwarakanath, K. S
dc.contributor.author	Shevgaonkar, R. K
dc.contributor.author	Sastry, Ch. V
dc.date.accessioned	2008-12-17T16:45:41Z
dc.date.available	2008-12-17T16:45:41Z
dc.date.issued	1982-06
dc.identifier.citation	Journal of Astrophysics and Astronomy, Vol. 3, pp. 207 - 216	en
dc.identifier.issn	0250- 6335
dc.identifier.uri	http://hdl.handle.net/2248/4106
dc.description	Open Access
dc.description.abstract	The results of observations of the two SNRs HB 9 and IC 443 are discussed. A map of HB 9 is presented whose main features are an elongation in the northerly direction and a strong region at the center of the map. The integrated flux density is 750 + or - 150 Jy at 34.5 MHz, and the spectral index is found to be constant in the range 34.5 to 2700 MHz. The shell structure of IC 443 was unresolved, and the integrated flux density is 440 + or - 88 Jy at 34.5 MHz. The spectral index in the frequency range from 20 to 10,700 MHz is -0.46 + or - 0.04.	en
dc.language.iso	en	en
dc.publisher	Indian Academy of Sciences	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1982JApA....3..207D	en
dc.relation.uri	http://www.springerlink.com/content/554trw5312l17nh2/	en
dc.rights	© Indian Academy of Sciences	en
dc.subject	Radio Astronomy	en
dc.subject	Supernova Remnants	en
dc.subject	Flux Density	en
dc.subject	Low Frequencies	en
dc.subject	Radio Spectra	en
dc.title	Observations of the supernova remnants HB 9 and IC 443 at 34.5 MHz	en
dc.type	Article	en