Superwind models for the dust shells around infrared carbon stars | Zendy

KyungWon Suh | Zendy

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Superwind models for the dust shells around infrared carbon stars

Author(s) -

KyungWon Suh

Publication year - 1997

Publication title -

monthly notices of the royal astronomical society

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 2.058

H-Index - 383

eISSN - 1365-8711

pISSN - 0035-8711

DOI - 10.1093/mnras/289.3.559

Subject(s) - physics , stars , astrophysics , carbon star , infrared , asymptotic giant branch , carbon fibers , astronomy , materials science , composite number , composite material

We investigate the observational effect of a superwind mass-loss phase driven by a thermal pulse in the interior of infrared carbon stars. We modify the dust density distribution by adding dust to form a region of enhanced density which proceeds outward. Depending on the position and the degree of the enhancement, the emergent model spectral energy distributions can be significantly different from...

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