Decametric radio spectra of some galaxies in clusters

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/948

Full metadata record

DC Field	Value	Language
dc.contributor.author	Subramanian, K. R	-
dc.contributor.author	Sastry, Ch. V	-
dc.date.accessioned	2006-04-11T08:34:23Z	-
dc.date.available	2006-04-11T08:34:23Z	-
dc.date.issued	1988-12	-
dc.identifier.citation	BASI, Vol. 16, No. 4, pp. 183-191	en
dc.identifier.uri	http://hdl.handle.net/2248/948	-
dc.description.abstract	Observations of 12 radio sources identified with clusters of galaxies were made in 1983-84 with a decameter-wave radio telescope. 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 between 34.5 MHz to 408 MHz is -1.32, much steeper than the average of extragalactic sources	en
dc.format.extent	248191 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Astronomical Society of Indian	en
dc.subject	Cluster of galaxies	en
dc.subject	Radio astronomy	en
dc.title	Decametric radio spectra of some galaxies in clusters	en
dc.type	Article	en
Appears in Collections:	BASI Publications

Files in This Item:

File	Description	Size	Format
SUBRAMANIAN.pdf		242.37 kB	Adobe PDF	View/Open

DSpace JSPUI