Spectrophotometry of comet West (1975n) after the perihelion passage

dc.contributor.author	Chaubey, U. S.
dc.date.accessioned	2011-11-11T10:53:47Z
dc.date.available	2011-11-11T10:53:47Z
dc.date.issued	1978
dc.identifier.citation	This article is downloaded from ADS article service	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/864
dc.description.abstract	In the wavelength range 350to 650 nm, the flux distribution of comet West (1975n) is presented for various dates following perihelion passage. The variations with heliocentric distances, in the flux of the emission features of the CN band at 388 nm, the C₂ bands at 474 nm, 516nm and 563 nm and NA at 589 nm, have been discussed. It is concluded that the comet was dust rich.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	ass54-233
dc.subject	Comet West (1975n)	en_US
dc.title	Spectrophotometry of comet West (1975n) after the perihelion passage	en_US
dc.type	Article	en_US