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ISO-SWS Spectra of AGB Stars
Authors:K Justtanont  I Yamamura  T De Jong  LBFM Waters
Institution:(1) SRON, PO Box 800, 9700 AV, Groningen, The Netherlands;(2) University of Amsterdam, Kruislaan 403, 1098 SJ Amsterdam, The Netherlands
Abstract:In this contribution, we present a few highlights of the guaranteed time program to observe AGB stars with differing chemical compositions and mass loss rates using ISO1 SWS. We briefly discuss C2H2 absorption in C-stars and O-rich stars with the 13 μm dust emission. This revised version was published online in September 2006 with corrections to the Cover Date.
Keywords:
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