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Dust driven mass loss from carbon stars as a function of stellar parameters - I. A grid of Solar-metallicity wind models

ASTRONOMY & ASTROPHYSICS, no. 1 (2010): 13

Cited: 61|Views23

Abstract

Context. Knowing how the mass loss of carbon-rich AGB stars depends on stellar parameters is crucial for stellar evolution modelling, as well as for the understanding of when and how circumstellar structures emerge around these stars, e.g., dust shells and so-called detached shells of expelled gas. Aims. The purpose of this paper is to ex...More

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