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 |