Unraveling the Dust Formation Process in R Dor
| Contribuinte(s) |
Lagadec, Eric Millour, F Lanz, T |
|---|---|
| Data(s) |
01/12/2015
|
| Resumo |
<p>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.</p> |
| Identificador |
http://dx.doi.org/10.1051/eas/1571057 http://www.scopus.com/inward/record.url?scp=84962318893&partnerID=8YFLogxK |
| Idioma(s) |
eng |
| Publicador |
EDP Sciences |
| Direitos |
info:eu-repo/semantics/restrictedAccess |
| Fonte |
Van De Sande , M , Decin , L , Lombaert , R , Walsh , C , Khouri , T , Li , X & Millar , T J 2015 , Unraveling the Dust Formation Process in R Dor . in E Lagadec , F Millour & T Lanz (eds) , EAS Publications Series . vol. 71-72 , EAS Publications Series , vol. 71-72 , EDP Sciences , pp. 255-257 , Physics of Evolved Stars Conference 2015 , Nice , France , 8-12 June . DOI: 10.1051/eas/1571057 |
| Palavras-Chave | #/dk/atira/pure/subjectarea/asjc/2200 #Engineering(all) |
| Tipo |
contributionToPeriodical |
