Abstract
1 ISO-SWS spectra of two Mira variables (R Cas and T Dra), taken at two different pulsational phases, are presented. We describe the reduction of the data and the encountered problems. The dust features observed by ISO at different phases and with the Low Resolution Spectrometer of IRAS are compared. We briefly discuss the results in terms of current models for the circumstellar dust shells of AGB variables.
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References
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© 1997 Springer Science+Business Media Dordrecht
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Hron, J., Loidl, R., Kerschbaum, F. (1997). Dust Features of Visually Bright AGB Variables as Seen by ISO and IRAS. 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_30
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DOI: https://doi.org/10.1007/978-94-017-1307-8_30
Publisher Name: Springer, Dordrecht
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