dc.contributor.author |
Mekkaden, M. V |
|
dc.date.accessioned |
2010-07-16T10:32:34Z |
|
dc.date.available |
2010-07-16T10:32:34Z |
|
dc.date.issued |
1985-12 |
|
dc.identifier.citation |
Astrophysics and Space Science, Vol. 117, No. 2, pp. 381-385 |
en |
dc.identifier.issn |
0004-640X |
|
dc.identifier.uri |
http://hdl.handle.net/2248/5203 |
|
dc.description.abstract |
The dependence of H-alpha emission strength on rotational period and spectral type in late-type stars is studied using published data. The emission strength shows strong correlation with rotation irrespective of age and spectral type. The chromospheric H-alpha emission strength in late-type dwarfs is a good diagnostic of rotation period in accordance with dynamo theory. |
en |
dc.language.iso |
en |
en |
dc.publisher |
Kluwer Academic Publishers |
en |
dc.relation.uri |
http://adsabs.harvard.edu/abs/1985Ap%26SS.117..381M |
en |
dc.rights |
© Kluwer Academic Publishers |
en |
dc.title |
Rotation and H-alpha emission activity in F8-G3 dwarfs |
en |
dc.type |
Article |
en |