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

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

2011-11-08

arxiv.org/abs/1111.2053v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

Scientific paper

We compute the mass and composition of dust produced by stars with masses in the range 1Msun

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