The infrared fluxes of early type stars

dc.contributor.author	Shylaja, B. S
dc.date.accessioned	2007-05-11T11:34:19Z
dc.date.available	2007-05-11T11:34:19Z
dc.date.issued	1994
dc.identifier.citation	BASI, Vol. 22, No. 1, pp. 35-45	en
dc.identifier.uri	http://hdl.handle.net/2248/1584
dc.description.abstract	It 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 studied	en
dc.format.extent	649340 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.subject	Early type stars	en
dc.subject	Stellar winds	en
dc.title	The infrared fluxes of early type stars	en
dc.type	Article	en