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

2011/11/08 by P. Ventura, M. Di Criscienzo, Ventura, P. +15
Physics and Astronomy · #Stellar, planetary, and galactic studies #Astronomy and Astrophysical Research #Gamma-ray bursts and supernovae

paper · pdf · doi:10.48550/arxiv.1111.2053

Abstract

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

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