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	2012-07-20T11:01:15Z
dc.date.available	2012-07-20T11:01:15Z
dc.date.issued	1982-06
dc.description	Open Access	en
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.identifier.citation	Journal of Astrophysics and Astronomy, 1982, Vol.3, p207	en
dc.identifier.issn	0250-6335
dc.identifier.issn	0973-7758 (Online)
dc.identifier.uri	http://hdl.handle.net/2289/5060
dc.language.iso	en	en
dc.publisher	Indian Academy of Sciences, Bangalore, India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1982JApA....3..207D	en
dc.rights	1982 Indian Academy of Sciences, Bangalore, India	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

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