Abstract
AGB stars are surrounded by cool circumstellar envelopes (CSEs) of gas and dust that are strong sources of IR thermal radiation.
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References
Busso M., Origlia L., Marengo M., Persi, P., Ferrari-Toniolo M., Silvestro, G., Corcione, L., Tapia, M., & Bohigas, J. 1996, A&A, in press
Marengo, M., Canil, G., Silvestro, G., Origlia, L., Busso, M., & Persi, P. 1996, in preparation
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© 1997 Springer Science+Business Media Dordrecht
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Marengo, M., Roseo, E., Silvestro, G., Busso, M., Persi, P. (1997). Near-IR Characterization of AGB Sources. In: Garzón, F., Epchtein, N., Omont, A., Burton, B., Persi, P. (eds) The Impact of Large Scale Near-IR Sky Surveys. Astrophysics and Space Science Library, vol 210. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-5784-1_32
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DOI: https://doi.org/10.1007/978-94-011-5784-1_32
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