Thursday, November 10, 2011

1111.2053 (P. Ventura et al.)

The transition from carbon dust to silicates production in low-metallicity AGB and SAGB stars    [PDF]

P. Ventura, M. Di Criscienzo, R. Schneider, R. Carini, R. Valiante, F. D'Antona, S. Gallerani, R. Maiolino, A. Tornambé
We compute the mass and composition of dust produced by stars with masses in the range 1MsunView original: http://arxiv.org/abs/1111.2053

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