C₂ in eta aquilae spectrum

dc.contributor.author	Bondal, K. R.
dc.contributor.author	Joshi, G. C.
dc.contributor.author	Pande, M. C.
dc.date.accessioned	2011-12-09T05:23:09Z
dc.date.available	2011-12-09T05:23:09Z
dc.date.issued	1973
dc.identifier.uri	http://hdl.handle.net/123456789/881
dc.description.abstract	The equivalent width of R₁ (16) line of the 0-0 band of the Swan system of C₂ calculated for the minimum phase of light variation in η Aql comes out to be 27 mÅ. Thus, if Dawe’s model atmosphere and the assumed abundance are realistic, the lines belonging to the 0-0 band of Swan system of C₂ will be observable in the η Aql spectrum.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	bac24-169
dc.subject	Eta Aquilae Spectrum	en_US
dc.title	C₂ in eta aquilae spectrum	en_US
dc.type	Article	en_US