An AGB Star with a Thick Circumstellar Shell

التفاصيل البيبلوغرافية
العنوان: An AGB Star with a Thick Circumstellar Shell
المؤلفون: Lifan Wang, Mark Durré, Syed Uddin, Jeremy Mould
سنة النشر: 2020
مصطلحات موضوعية: 010504 meteorology & atmospheric sciences, Red giant, Shell (structure), FOS: Physical sciences, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Star (graph theory), 01 natural sciences, 0103 physical sciences, Asymptotic giant branch, Astrophysics::Solar and Stellar Astrophysics, Oxygen rich, Large Magellanic Cloud, 010303 astronomy & astrophysics, Solar and Stellar Astrophysics (astro-ph.SR), Astrophysics::Galaxy Astrophysics, 0105 earth and related environmental sciences, Physics, Astronomy and Astrophysics, Astrophysics - Astrophysics of Galaxies, Galaxy, Stars, Astrophysics - Solar and Stellar Astrophysics, Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), Astrophysics::Earth and Planetary Astrophysics
الوصف: 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.
6 pages, 5 figures, accepted for publication in PASP
اللغة: English
URL الوصول: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d294723da693b19aeaad13bf5a428f88
http://arxiv.org/abs/2002.08588
حقوق: OPEN
رقم الأكسشن: edsair.doi.dedup.....d294723da693b19aeaad13bf5a428f88
قاعدة البيانات: OpenAIRE