IRAS observations of R Cor Bor stars

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3885

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DC Field	Value	Language
dc.contributor.author	Kameswara Rao, N	-
dc.contributor.author	Nandy, K	-
dc.date.accessioned	2008-09-24T14:48:47Z	-
dc.date.available	2008-09-24T14:48:47Z	-
dc.date.issued	1986-09	-
dc.identifier.citation	Monthly Notices of Royal Astronomical Society, Vol. 222, No. 2, pp. 357 - 364	en
dc.identifier.issn	0035-8711	-
dc.identifier.uri	http://hdl.handle.net/2248/3885	-
dc.description.abstract	The IRAS observations of R Cr B, SU Tau and V 348 Sgr indicate the existence of a cool dust component of temperature about 30 K in R Cr B and SU Tau and less than or equal to 100 K in V 348 Sgr, in addition to the hot dust. It is suggested that this cool dust shell is a remnant of the stage when these stars were red giants for the first time. Although R Cr B was observed by IRAS during a visual light minimum no significant IR flux increase was apparent.	en
dc.language.iso	en	en
dc.publisher	Royal Astronomical Society	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1986MNRAS.222..357K	en
dc.subject	Infrared astronomy satellite	en
dc.subject	Spaceborne astronomy	en
dc.subject	Stellar evolution	en
dc.subject	Stellar spectrophotometry	en
dc.subject	Stellar temperature	en
dc.subject	Variable stars	en
dc.subject	Cosmic dust	en
dc.subject	Red giant stars	en
dc.subject	Stellar envelopes	en
dc.title	IRAS observations of R Cor Bor stars	en
dc.type	Article	en
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