On the radii of Ap and Am stars

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4179

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DC Field	Value	Language
dc.contributor.author	Babu, G. S. D	-
dc.contributor.author	Shylaja, B. S	-
dc.date.accessioned	2008-12-29T11:57:41Z	-
dc.date.available	2008-12-29T11:57:41Z	-
dc.date.issued	1983-01	-
dc.identifier.citation	Astrophysics and Space Science, Vol. 89, No. 2, pp. 341 - 344	en
dc.identifier.issn	0004-640X	-
dc.identifier.uri	http://hdl.handle.net/2248/4179	-
dc.description	Open Access	-
dc.description.abstract	The radii of several Ap and Am stars have been compared with those of the normal A stars of the main sequence. Though the brighter Ap stars have a little larger radii than the main sequence stars, they may not be much different from those of the slightly evolved normal A stars. The Am stars have radii with which they appear to be merging with those of cooler A stars of the main sequence. The Ap stars have radii predominantly in the range of 1.8 to 3.4 solar radii, while the Am stars are mainly concentrated between 1.8 and 2.2 solar radii.	en
dc.language.iso	en	en
dc.publisher	D. Reidel Publishing Co.	en
dc.relation.uri	http://dx.doi.org/10.1007/BF00655986	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1983Ap%26SS..89..341B	en
dc.subject	A Stars	en
dc.subject	Magnetic Stars	en
dc.subject	Peculiar Stars-Radii	en
dc.subject	S Stars	en
dc.subject	Stellar Magnitude	en
dc.title	On the radii of Ap and Am stars	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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