The transition from carbon dust to silicate production in low-metallicity asymptotic giant branch and super-asymptotic giant branch stars
Article first published online: 8 DEC 2011
© 2011 The Authors Monthly Notices of the Royal Astronomical Society © 2011 RAS
Monthly Notices of the Royal Astronomical Society
Volume 420, Issue 2, pages 1442–1456, February 2012
How to Cite
Ventura, P., Di Criscienzo, M., Schneider, R., Carini, R., Valiante, R., D’Antona, F., Gallerani, S., Maiolino, R. and Tornambé, A. (2012), The transition from carbon dust to silicate production in low-metallicity asymptotic giant branch and super-asymptotic giant branch stars. Monthly Notices of the Royal Astronomical Society, 420: 1442–1456. doi: 10.1111/j.1365-2966.2011.20129.x
- Issue published online: 24 JAN 2012
- Article first published online: 8 DEC 2011
- Accepted 2011 November 3. Received 2011 November 2; in original form 2011 July 31
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