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 ISO 1 SWS. We briefly discuss C2H2 absorption in C-stars and 0-rich stars with the 13 μm dust emission.
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© 1997 Springer Science+Business Media Dordrecht
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Justtanont, K., Yamamura, I., De Jong, T., Waters, L.B.F.M. (1997). ISO-SWS Spectra of AGB Stars. In: Cherchneff, I., Millar, T.J. (eds) Dust and Molecules in Evolved Stars. Springer, Dordrecht. https://doi.org/10.1007/978-94-017-1307-8_3
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DOI: https://doi.org/10.1007/978-94-017-1307-8_3
Publisher Name: Springer, Dordrecht
Print ISBN: 978-90-481-5018-2
Online ISBN: 978-94-017-1307-8
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