The transition from carbon dust to silicate production in low-metallicity asymptotic giant branch and super-asymptotic giant branch stars-Reference-Cited by-同舟云学术

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The transition from carbon dust to silicate production in low-metallicity asymptotic giant branch and super-asymptotic giant branch stars

Published:2011-12-08 Issue:2 Volume:420 Page:1442-1456
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Ventura P.,Di Criscienzo M.,Schneider R.,Carini R.,Valiante R.,D’Antona F.,Gallerani S.,Maiolino R.,Tornambé A.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/420/2/1442/3071161/mnras0420-1442.pdf

Reference66 articles.

1. A compilation of charged-particle induced thermonuclear reaction rates

2. Using FU Orionis outbursts to constrain self-regulated protostellar disk models

3. Dust formation and survival in supernova ejecta

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