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Dust shell around F and G Main-Sequence stars
Authors:B S Rautela  B B Sanwal  G C Joshi
Institution:(1) Uttar Pradesh State Observatory, Manora Peak, Naini Tal, India
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 lsquoVega-likersquo 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 lsquoVega-likersquo and the equilibrium distances of dust shells are within the planet-forming region.
Keywords:
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