On the observability of CO and CO⁺ in eta aquilae

dc.contributor.author	Pande, M. C.
dc.contributor.author	Joshi, G. C.
dc.date.accessioned	2011-12-15T04:42:31Z
dc.date.available	2011-12-15T04:42:31Z
dc.date.issued	1972
dc.identifier.uri	http://hdl.handle.net/123456789/882
dc.description.abstract	The equivalent widths of R(29) line belonging to 0-2 in η Aql are found to be 0.200 m Å and 4.17 m Å and of R(31) m Å at maximum and minimum phases respectively. Thus if Dawe’s model atmospheres are realistic there is some chance of detecting the lines of the first overtone of CO near minimum phase light variation in the star.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	bac24-171
dc.subject	Eta Aquilae	en_US
dc.title	On the observability of CO and CO⁺ in eta aquilae	en_US
dc.type	Article	en_US