The colors of Am Stars

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4627

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DC Field	Value	Language
dc.contributor.author	Shylaja, B. S	-
dc.contributor.author	Babu, G. S. D	-
dc.date.accessioned	2009-07-11T12:10:44Z	-
dc.date.available	2009-07-11T12:10:44Z	-
dc.date.issued	1993-01	-
dc.identifier.citation	M.M. Dworetsky, F. Castelli, R. Faraggiana., eds., Peculiar versus Normal Phenomena in A-type and Related Stars. International Astronomical Union, Colloquium No. 138, ASP Conference series Vol. 44 held in Trieste, Italy, July 1992, pp. 203 - 207	en
dc.identifier.isbn	0937707635	-
dc.identifier.uri	http://hdl.handle.net/2248/4627	-
dc.description	Open Access	-
dc.description.abstract	The energy distribution of the Am stars are affected by the line blanketing, which appears as a deviation in the behaviour of color indices with reference to the normal stars. In this paper we study the various color indices along with the data from IRAS and try to identify a realistic representative of the effective temperature. An excess in the IR also becomes apparent in same cases.	en
dc.language.iso	en	en
dc.publisher	Astronomical Society of the Pacific	en
dc.relation.ispartofseries	Astronomical Society of the Pacific Conference series;Vol. 44	-
dc.relation.ispartofseries	IAU Colloquium;No.138	-
dc.relation.uri	http://adsabs.harvard.edu/abs/1993ASPC...44..203S	en
dc.rights	© Astronomical Society of the Pacific	-
dc.subject	Peculiar Stars	en
dc.subject	Stars	en
dc.title	The colors of Am Stars	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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