Chemistry in the circumstellar medium. Unveiling the dust formation zone

Details Chemistry in the circumstellar medium. Unveiling the dust formation zone Chemistry in the circumstellar medium. Unveiling the dust formation zone

Jan 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ap%26ss.313..223m&link_type=abstract

Astrophysics and Space Science, Volume 313, Issue 1-3, pp. 223-227

Astronomy and Astrophysics

Astrophysics

Circumstellar Envelopes, Agb Stars, Astrochemistry

Scientific paper

The growth of dust grains in the inner regions of late-type stars is shrouded in mystery due to the difficulty of understanding the growth of heterogeneous particles from simple atoms and molecules and the lack of observational data. This article reviews the molecular processes important in circumstellar envelopes and discusses how ALMA might be used to probe the dust formation zone either directly or indirectly.

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