1. IIA Institutional Repository
  2. Publications of Astronomical Society of India
  3. BASI Publications
Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2503
Full metadata record
DC FieldValueLanguage
dc.contributor.authorShylaja, B. S-
dc.contributor.authorAshok, N. M-
dc.date.accessioned2008-06-25T10:07:21Z-
dc.date.available2008-06-25T10:07:21Z-
dc.date.issued2002-
dc.identifier.citationBASI, Vol. 30, No. 2, pp. 491 - 500en
dc.identifier.urihttp://hdl.handle.net/2248/2503-
dc.description.abstractThe 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.extent743474 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2002BASI...30..491Sen
dc.subjectAm Starsen
dc.subjectChemically Peculiar Starsen
dc.subjectEnergy Distributionen
dc.subjectInfrared Fluxesen
dc.titleIR observations of Am starsen
dc.typeArticleen
Appears in Collections:BASI Publications

Files in This Item:
File Description SizeFormat 
shyalajabs.pdf726.05 kBAdobe PDFThumbnail
View/Open
Show simple item record


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.