Abstract
1 Exploratory synthetic spectra were computed for carbon-rich long-period variables. We used dynamic model atmospheres of Höfner & Dorfi (1997) and calculated partial pressures, absorption- and scattering coefficients as input for the spectral synthesis code of Jorgensen et al. (1992). First ISO SWS-observations of the carbon-Mira T Dra are compared with our synthetic spectra.
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References
Höfner, S., Dorfi, E. A., 1997, AandA, 319, 648
Jorgensen, U.G., Johnson, H.R., Nordlund, A, 1992, AandA, 261, 263
Kerschbaum, F., Hron, J., 1996, AandA, 308, 489
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© 1997 Springer Science+Business Media Dordrecht
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Loidl, R., Hron, J., Aringer, B., Kerschbaum, F., Höfner, S., Jørgensen, U.G. (1997). Synthetic Spectra of Long-Period Variables: A First Comparison with ISO Observations. 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_38
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DOI: https://doi.org/10.1007/978-94-017-1307-8_38
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