Effective temperatures, radii and bolometric magnitudes of Ap and Am stars

dc.contributor.author	Babu, G. S. D.
dc.contributor.author	Rautela, B. S.
dc.date.accessioned	2011-11-11T05:39:17Z
dc.date.available	2011-11-11T05:39:17Z
dc.date.issued	1978
dc.identifier.citation	This article is downloaded from ADS article service	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/860
dc.description.abstract	The effective temperatures, radii and bolometric magnitudes of Ap, Am and normal A stars have been estimated from their energy distribution curves between 478 nm and 680 nm. All the Am stars and one Ap star (i.e. β CrB) were found to be affected by line blanketing, a rough estimation of which in the respective (B-V) colours has been found out in each case.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	ass59-245
dc.subject	Ap and Am stars	en_US
dc.title	Effective temperatures, radii and bolometric magnitudes of Ap and Am stars	en_US
dc.type	Article	en_US