2 resultados para Dor Crônica Diagnóstico
em QUB Research Portal - Research Directory and Institutional Repository for Queen's University Belfast
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>