Dust around Herbig Ae/Be stars: IRAS low resolution spectra

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1550

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DC Field	Value	Language
dc.contributor.author	Bhatt, H. C	-
dc.contributor.author	Gorti, U	-
dc.date.accessioned	2007-05-09T06:01:25Z	-
dc.date.available	2007-05-09T06:01:25Z	-
dc.date.issued	1993	-
dc.identifier.citation	BASI, Vol. 21, pp. 541-544	en
dc.identifier.uri	http://hdl.handle.net/2248/1550	-
dc.description.abstract	IRAS low resolution spectra are presented for 17 Herbig Ae/Be stars. The observed spectral characteristics are correlated with reddening E(B-V) and the spectral type of the star. The silicate emission feature at 9.7 micrometers is found only in the spectra of Herbig Ae/Be stars with E(B-V) less than or = 1.0 and spectral type later than approximately A0 while this feature is in absorption in stars with E(B-V) less than or = 1.0 and spectral type either than approximately A0. The unidentified emission feature at 11.3 micrometers is found in the spectra of stars with spectral type earlier than approximately A0. These observations are interpreted in terms of the composition of dust in the circumstellar environments of Herbig Ae/Be stars.	en
dc.format.extent	265289 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.subject	Herbig	en
dc.subject	Star dust	en
dc.title	Dust around Herbig Ae/Be stars: IRAS low resolution spectra	en
dc.type	Article	en
Appears in Collections:	BASI Publications

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