Occultation of Sgr A

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DC Field	Value	Language
dc.contributor.author	Krishna, G.	-
dc.contributor.author	Swarup, G.	-
dc.contributor.author	Sarma, N.V.G.	-
dc.contributor.author	Joshi, M.N.	-
dc.date.accessioned	2012-08-06T09:08:28Z	-
dc.date.available	2012-08-06T09:08:28Z	-
dc.date.issued	1972	-
dc.identifier.citation	Nature, 1972, Vol.239, p5367	en
dc.identifier.issn	0028-0836	-
dc.identifier.issn	1476-4687(Online)	-
dc.identifier.uri	http://hdl.handle.net/2289/5189	-
dc.description	Restricted Access.	en
dc.description.abstract	INTERFEROMETRIC1,2 and lunar occultation3-5 observations show that the radio source Sgr A, which is located near the galactic centre, consists of several components varying in size from a few arc s to a few arc min. Lunar occultation observations made at Ootacamund on September 9, 1970, have provided detailed information on the structure of the source of 327 MHz and have revealed the presence of an extended component 10 × 4 arc min in size and centred approximately on Sgr A. The extended source has an inclination of 45° +/- 15° to the galactic plane, similar to that of the 20 cm continuum ridges6.	en
dc.language.iso	en	en
dc.publisher	Nature Publishing Group	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1972Natur.239...91K	en
dc.relation.uri	http://dx.doi.org/10.1038/239091a0	en
dc.rights	1972 Nature Publishing Group	en
dc.title	Occultation of Sgr A	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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