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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/5060
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dc.contributor.authorDwarakanath, K.S.-
dc.contributor.authorShevgaonkar, R.K.-
dc.contributor.authorSastry, Ch.V.-
dc.date.accessioned2012-07-20T11:01:15Z-
dc.date.available2012-07-20T11:01:15Z-
dc.date.issued1982-06-
dc.identifier.citationJournal of Astrophysics and Astronomy, 1982, Vol.3, p207en
dc.identifier.issn0250-6335-
dc.identifier.issn0973-7758 (Online)-
dc.identifier.urihttp://hdl.handle.net/2289/5060-
dc.descriptionOpen Accessen
dc.description.abstractThe 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.isoenen
dc.publisherIndian Academy of Sciences, Bangalore, Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/1982JApA....3..207Den
dc.rights1982 Indian Academy of Sciences, Bangalore, Indiaen
dc.subjectradio astronomyen
dc.subjectsupernova remnantsen
dc.subjectflux densityen
dc.subjectlow frequenciesen
dc.subjectradio spectraen
dc.titleObservations of the supernova remnants HB 9 and IC 443 at 34.5 MHzen
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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