Dust formation and wind acceleration around the aluminum oxide–rich AGB star W Hydrae

Dust grains, formed around asymptotic giant branch (AGB) stars, are accelerated by stellar radiation to drive stellar winds, which supply freshly synthesized nuclides to the Galaxy. Silicate is the dominant dust species in space, but ~40% of oxygen-rich AGB stars are thought to have comparable amoun...

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Detalles Bibliográficos
Autores principales: Takigawa, Aki, Kamizuka, Takafumi, Tachibana, Shogo, Yamamura, Issei
Formato: Online Artículo Texto
Lenguaje:English
Publicado: American Association for the Advancement of Science 2017
Materias:
Research Articles
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5665597/
https://www.ncbi.nlm.nih.gov/pubmed/29109978
http://dx.doi.org/10.1126/sciadv.aao2149

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5665597/
https://www.ncbi.nlm.nih.gov/pubmed/29109978
http://dx.doi.org/10.1126/sciadv.aao2149

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