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Circumstellar Dust
https://doi.org/10.1142/9789812567666_0006Cited by:0 (Source: Crossref)
Abstract:
The following sections are included:
Introduction
AGB Stars
Mass Loss from Stars
Theoretical Considerations
Dust Formation
Condensation of Dust
C/O < 1 (Oxygen-rich stars)
C/O > 1 (Carbon-rich stars)
C/O = 1 (S-Stars)
Circumstellar Chemistry
Observational Results
Carbon-rich Stars
Oxygen-rich Stars
S Stars
UIR Bands in Oxygen-rich Supergiants
Stars of Other Type
Herbig Ae/Be Stars
Vega-Type Stars
Planetary Nebulae
Novae
Supernovae
References
