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An AGB Star with a Thick Circumstellar Shell

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arxiv 2002.08588 v1 pith:E5ELG4QN submitted 2020-02-20 astro-ph.SR astro-ph.GA

Jeremy Mould , Mark Durré , Syed Uddin , Lifan Wang This is my paper · ORCID
classification astro-ph.SRastro-ph.GA
keywords stargiantmassshellasymptoticblack-bodybranchcenter
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The Asymptotic Giant Branch (AGB) is the terminal phase of red giant evolution with timescales of millions of years and a total mass lost from the star that is a significant fraction of the initial mass. Investigation of one of these stars, WISEA J173046.10-344455.5, a kpc in the direction of the center of the Galaxy, reveals a cool oxygen rich star with a dust shell of black-body temperature 1305 K.

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