Dusty shells surrounding the carbon variables S Scuti and RT Capricorni

M. Mečina; F. Kerschbaum; M. A. T. Groenewegen; R. Ottensamer; J. A. D. L. Blommaert; A. Mayer; L. Decin; A. Luntzer; B. Vandenbussche; Th. Posch; C. Waelkens

doi:10.1051/0004-6361/201321117

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Volume 566 (June 2014)

A&A, 566 (2014) A69

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Fig. 9

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Top: SED of the RT Cap model fit compared with the photometric data (for references see Table 3), part of an LRS spectrum was also taken into account. Bottom: comparison between the LRS (solid line) and the model spectrum. The SiC feature in the model is narrower than observed.

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