Abstract
Modelling the spectral energy distribution (SED) of asymptotic giant branch (AGB) stars is one of the most important diagnostic tools to study the chemical composition of the cosmic dust grains. The extended circumstellar envelopes around AGB stars are places of dust formation and important sources of recycled interstellar matter.
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© 1997 Springer Science+Business Media Dordrecht
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Bagnulo, S., Doyle, J.G. (1997). Observations and Modelling of Spectral Energy Distributions of Asymptotic Giant Branch 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_22
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DOI: https://doi.org/10.1007/978-94-017-1307-8_22
Publisher Name: Springer, Dordrecht
Print ISBN: 978-90-481-5018-2
Online ISBN: 978-94-017-1307-8
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