Simulating Chemical Abundances in the Circumstellar Nebula of the Late Stage Binary RY Scuti

Simulating Chemical Abundances in the Circumstellar Nebula of the Late Stage Binary RY Scuti

RY Scuti, thought to be a Wolf–Rayet (WR) progenitor, is a massive post-main-sequence binary star system undergoing Roche-lobe overflow (RLOF). SOFIA (+FORCAST) spectroscopy of the inner, ionized region of RY Scuti’s double ringed toroidal nebula affirms the previous detection of the well-studied 12...

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Bibliographic Details
Main Authors: Sarah H. Taft, Robert D. Gehrz, Charles E. Woodward, Nathan Smith, Isabelle Perron, Annalisa Citro
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astronomical Journal
Subjects:
Binary stars
Chemical abundances
Stellar atmospheres
Online Access:https://doi.org/10.3847/1538-3881/adc251
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https://doi.org/10.3847/1538-3881/adc251

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