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Decametric radio spectra of some galaxies in clusters

dc.contributor.authorSubramanian, K.R.
dc.contributor.authorSastry, Ch.V.
dc.date.accessioned2006-06-12T10:49:47Z
dc.date.available2006-06-12T10:49:47Z
dc.date.issued1989
dc.description.abstractObservations of 12 radio sources identified with clusters of galaxies were made 1983-84 with the decameter wave radio telescope at Gauribidanur. The measured flux densities at 34.5 MHz are combined with other low frequency measurements to derive their radio spectra. It is found that the average spectral index in the frequency range 34.5 MHz to 408 MHz is -1.32, much steeper than the average of extragalactic sources.en
dc.format.extent183214 bytes
dc.format.mimetypeapplication/pdf
dc.identifier.citationBulletin of the Astronomical Society of India, 1989, Vol.16, p183-191en
dc.identifier.issn0304-9523
dc.identifier.urihttp://hdl.handle.net/2289/1359
dc.language.isoenen
dc.publisherThe Astronomical Society of Indiaen
dc.rights(1989) by the Astronomical Society of India.en
dc.subjectCluster of galaxiesen
dc.subjectRadio astronomyen
dc.titleDecametric radio spectra of some galaxies in clustersen
dc.typeArticleen

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