dc.contributor.author | Mallik, S. G. V | |
dc.date.accessioned | 2008-09-06T17:01:28Z | |
dc.date.available | 2008-09-06T17:01:28Z | |
dc.date.issued | 1998 | |
dc.identifier.citation | BASI, Vol. 26, pp. 479 - 492 | en |
dc.identifier.uri | http://hdl.handle.net/2248/3447 | |
dc.language.iso | en | en |
dc.publisher | Astronomical Society of India | en |
dc.relation.uri | http://adsabs.harvard.edu/abs/1998BASI...26..479M | en |
dc.subject | Cool Stars | en |
dc.subject | Chromospheric Activity | en |
dc.subject | Lithium Abundance | en |
dc.title | The central depth of the Ca II triplet lines as a discriminant of chromospheric activity in late type stars | en |
dc.type | Article | en |