Spectrophotometry of comet Austin (1982g) during post perihelion period

dc.contributor.author	Goraya, P. S.
dc.contributor.author	Rautela, B. S.
dc.contributor.author	Sanwal, B. B.
dc.date.accessioned	2010-07-27T06:37:58Z
dc.date.available	2010-07-27T06:37:58Z
dc.date.issued	1984
dc.identifier.citation	This article downloded from ADS Free Online Journal	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/711
dc.description.abstract	Spectrum scans have been obtained of the head of Comet Austin on six nights at heliocentric distances (r) from 0.70 to 0.87 AU. The useful spectral region is λλ330-750 nm. Strong emission features of CN (388nm) and Swan band sequence of C₂ (474, 516, and 563 nm) were identified. Weak emission features of CH+C₂ (436nm), C₂ (600nm), CN (420nm) and CH+C₃ (405 nm) have also been found present. There is a change in the ratio of CN (388nm) to C₂ (516 nm) emission strength with increasing heliocentric distance. An estimate of the CN and C₂ abundances has been made and their production rates have been derived.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	emp30-63
dc.subject	Comet Austin (1982g)	en_US
dc.title	Spectrophotometry of comet Austin (1982g) during post perihelion period	en_US
dc.type	Article	en_US