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Inner radii of dust shells and stellar diameters obtained by an infrared stellar interferometer at 11 micron wavelength
Authors:W C Danchi  M Bester  L J Greenhill  C G Degiacomi  N Geis  D Hale  B Lopez  C H Townes
Institution:(1) Space Sciences Laboratory, University of California, 94720-7450 Berkeley, CA, USA;(2) Present address: Center for Astrophysics, 60 Garden St., 02138 Cambridge, MA, USA;(3) I. Physikalisches Institut, Universität zu Köln, D-50937 Köln, Germany;(4) Physics Department, University of Pittsburgh, 15260 Pittsburgh, PA, USA;(5) Observatoire de la Côte d'Azur, Nice cedex 4, 06304, France
Abstract:Visibility data and analyses are discussed for 16 late-type stars observed with the Infrared Spatial Interferometer (ISI) of the University of California, Berkeley.
Keywords:interferometry  mass loss  dust shells  stellar diameters  masers
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