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. TornambéWe compute the mass and composition of dust produced by stars with masses in the range 1MsunView original: http://arxiv.org/abs/1111.2053
No comments:
Post a Comment