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/2248/3447
Full metadata record
DC FieldValueLanguage
dc.contributor.authorMallik, S. G. V-
dc.date.accessioned2008-09-06T17:01:28Z-
dc.date.available2008-09-06T17:01:28Z-
dc.date.issued1998-
dc.identifier.citationBASI, Vol. 26, pp. 479 - 492en
dc.identifier.urihttp://hdl.handle.net/2248/3447-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/1998BASI...26..479Men
dc.subjectCool Starsen
dc.subjectChromospheric Activityen
dc.subjectLithium Abundanceen
dc.titleThe central depth of the Ca II triplet lines as a discriminant of chromospheric activity in late type starsen
dc.typeArticleen
Appears in Collections:BASI Publications

Files in This Item:
File Description SizeFormat 
Mallik SV.pdf911.02 kBAdobe PDFThumbnail
View/Open
Show simple item record


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