Spectrophotometry of comet Bennett

dc.contributor.author	Babu, G. S. D.
dc.contributor.author	Saxena, P. P.
dc.date.accessioned	2012-01-04T10:50:26Z
dc.date.available	2012-01-04T10:50:26Z
dc.date.issued	1972
dc.identifier.uri	http://hdl.handle.net/123456789/896
dc.description.abstract	Phtotoelectric spectrum scans of the head of comet Bennett (1969i) covering the range 352÷612 mμ are presented and the emission features of CN, CH, C₂ and Na have been identified. The scattered light becomes redder as the phase angle decreases and matches with the solar light scattered according to the λ² law at a particular phase angle indicating that the size of the scattering particles is of the order of 0.5 μ.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	bac23-346
dc.subject	Comet Bennett, Spectrophotometry	en_US
dc.title	Spectrophotometry of comet Bennett	en_US
dc.type	Article	en_US