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/2248/1584
Full metadata record
DC FieldValueLanguage
dc.contributor.authorShylaja, B. S-
dc.date.accessioned2007-05-11T11:34:19Z-
dc.date.available2007-05-11T11:34:19Z-
dc.date.issued1994-
dc.identifier.citationBASI, Vol. 22, No. 1, pp. 35-45en
dc.identifier.urihttp://hdl.handle.net/2248/1584-
dc.description.abstractIt is well known that the strong winds of the early type stars modify the fluxes in the infrared and radio wavelength regions. This aspect has been used here to explain the infrared fluxes by the method of 'curve of growth'. Further, it has also been used to derive the excess flux at 3.6 micrometers, 4.8 micrometers and 12 micrometers and compared with observations. The effect of introducing a temperature gradient in the wind has also been studieden
dc.format.extent649340 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectEarly type starsen
dc.subjectStellar windsen
dc.titleThe infrared fluxes of early type starsen
dc.typeArticleen
Appears in Collections:BASI Publications

Files in This Item:
File Description SizeFormat 
Paper_3.pdf634.12 kBAdobe PDFThumbnail
View/Open
Show simple item record


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