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Modelling the Dust Around Vega-Like StarsModels are presented of four Vega-like stars: main-sequence stars with infrared emission from circumstellar dust. The dusty environments of the four stars are rather diverse, as shown by their spectral energy distributions. Good fits to the observations were obtained for all four stars.
Document ID
19970007823
Acquisition Source
Ames Research Center
Document Type
Conference Paper
Authors
Sylvester, Roger J. (University Coll. London, United Kingdom)
Skinner, C. J. (Space Telescope Science Inst. Baltimore, MD United States)
Barlow, M. J. (University Coll. London, United Kingdom)
Date Acquired
August 17, 2013
Publication Date
October 1, 1996
Publication Information
Publication: From Stardust to Planetesimals: Contributed Papers
Subject Category
Astronomy
Accession Number
97N14444
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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IDRelationTitle19970007821Collected WorksFrom Stardust to Planetesimals: Contributed Papers
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