Evolved Massive Stars at Low Metallicity. VI. Mass-loss Rate of Red Supergiant Stars in the Large Magellanic Cloud

Mass loss is a crucial process that affects the observational properties, evolution path, and fate of highly evolved stars. However, the mechanism of mass loss is still unclear, and the mass-loss rate (MLR) of red supergiant stars (RSGs) requires further research and precise evaluation. To address t...

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Bibliographic Details

Published in:	The Astronomical Journal
Main Authors:	Jing Wen, Jian Gao, Ming Yang, Bingqiu Chen, Yi Ren, Tianding Wang, Biwei Jiang
Format:	Article
Language:	English
Published:	IOP Publishing 2024-01-01
Subjects:	Red supergiant stars Stellar mass loss Circumstellar dust Large Magellanic Cloud Interstellar medium
Online Access:	https://doi.org/10.3847/1538-3881/ad12bf