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The 69-μm forsterite band as a dust temperature indicator
Authors:J. E.Bowey  M. J.Barlow  F. J.Molster  A. M.Hofmeister  C.Lee  C.Tucker  T.Lim  P. A. R.Ade  L. B. F. M.Waters
Affiliation:1Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT; 2ESTEC/ESA, RSSD-ST, Keplerlaan 1, 2201 AZ Noordwijk, the Netherlands; 3Department of Earth and Planetary Science, Washington University, Box 1169, 1 Brookings Drive, St Louis, MO 63130, USA; 4Department of Physics and Astronomy, University of Wales, Cardiff, 5 The Parade, Cardiff CF24 3YB; 5Space Science Department, Rutherford Appleton Laboratory, Chilton, Didcot OX11 0QX; 6Astronomical Institute, University of Amsterdam, Kruislaan 403, 1098 SJ Amsterdam, the Netherlands
Abstract:
Keywords:line: identification    stars: AGB and post-AGB    circumstellar matter    stars: pre-main-sequence    dust, extinction    infrared: general
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