IR observations of Am stars

dc.contributor.author	Shylaja, B. S
dc.contributor.author	Ashok, N. M
dc.date.accessioned	2008-06-25T10:07:21Z
dc.date.available	2008-06-25T10:07:21Z
dc.date.issued	2002
dc.identifier.citation	BASI, Vol. 30, No. 2, pp. 491 - 500	en
dc.identifier.uri	http://hdl.handle.net/2248/2503
dc.description.abstract	The IR observations of chemically peculiar stars are carried out and compared with the previous data in IR and far IR from IRAS. The flux redistribution appears to be a common phenomenon in all the stars of this class. The observed energy distribution and a model fit based on effective temperature estimates show slight excess in the IR.	en
dc.format.extent	743474 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/2002BASI...30..491S	en
dc.subject	Am Stars	en
dc.subject	Chemically Peculiar Stars	en
dc.subject	Energy Distribution	en
dc.subject	Infrared Fluxes	en
dc.title	IR observations of Am stars	en
dc.type	Article	en