Rotation and H-alpha emission activity in F8-G3 dwarfs

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5203

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DC Field	Value	Language
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
Appears in Collections:	IIAP Publications

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