1. IIA Institutional Repository
  2. Publications of Astronomical Society of India
  3. BASI Publications
Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1477
Full metadata record
DC FieldValueLanguage
dc.contributor.authorSubrahmanyam, P. V-
dc.contributor.authorRaghavender Rao, C-
dc.contributor.authorSreedhar Rao, S-
dc.date.accessioned2007-04-13T11:18:16Z-
dc.date.available2007-04-13T11:18:16Z-
dc.date.issued1993-03-
dc.identifier.citationBASI, Vol. 21, No. 1, pp 63-65en
dc.identifier.urihttp://hdl.handle.net/2248/1477-
dc.description.abstractSpectroscopic observations of the long period variable epsilon Aurigae were made during its 1982-84 eclipse. It is found that the Ca II H and K lines show variation in their equivalent widths. The equivalent widths of these lines are larger before and after totality compared with that during totality. This phenomenon may be due to the atmospheric effect of the secondaryen
dc.format.extent206255 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectLong period eclipsing variableen
dc.subjectEquivalent widthsen
dc.titleA note on the spectra of epsilon Aurigaeen
dc.typeArticleen
Appears in Collections:BASI Publications

Files in This Item:
File Description SizeFormat 
paper_5.pdf201.42 kBAdobe PDFThumbnail
View/Open
Show simple item record


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.