Dust shell around F and G main-sequence stars

dc.contributor.author	Rautela, B. S.
dc.contributor.author	Sanwal, B. B.
dc.contributor.author	Joshi, G. C.
dc.date.accessioned	2010-02-01T05:57:07Z
dc.date.available	2010-02-01T05:57:07Z
dc.date.issued	1990
dc.identifier.citation	This article downloded from ADS Free Online Journal	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/475
dc.description.abstract	One-hundred and three nearby bright Main-Sequence stars of spectral type F and G have been searched for infrared excess in order to find out 'Vega-like' characteristics. In our sample of bright Main-Sequence F and G stars none of the G-type stars show infrared excess but 4 out of 28 F-type stars are 'Vega-like' and the equilibrium distances of dust shells are within the planet-forming region.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	ass166-13
dc.subject	F & G - main sequence stars	en_US
dc.title	Dust shell around F and G main-sequence stars	en_US
dc.type	Article	en_US