Unraveling The Dust Formation Process In R DOR
Paper i proceeding, 2015

Using both dynamical and chemical modelling, we derive an accurate abundance profile for the molecule SiO in the stellar wind of R Dor, an O-rich AGB star. SiO plays a key role in the dust formation process in O-rich AGB stars. This method will be applied to additional molecules, with the aim to achieve a detailed overview of the molecular abundance pattern in the wind of R Dor.

agb

chemistry

stars

Författare

M. Van De Sande

KU Leuven

L. Decin

KU Leuven

Robin Lombaert

Chalmers, Rymd- och geovetenskap, Onsala rymdobservatorium

C. Walsh

Universiteit Leiden

Theo Khouri

Chalmers, Rymd- och geovetenskap, Radioastronomi och astrofysik

X. Li

Universiteit Leiden

T.J. Millar

Queen's University Belfast

EAS Publications Series

1633-4760 (ISSN) 1638-1963 (eISSN)

Vol. 71-72 255-257

Ämneskategorier

Astronomi, astrofysik och kosmologi

Fundament

Grundläggande vetenskaper

DOI

10.1051/eas/1571057

ISBN

978-2-7598-1907-2