Mass-loss Rate of Highly Evolved Stars in the Magellanic Clouds

Asymptotic giant branch stars (AGBs) and red supergiant stars (RSGs) exhibit significant mass-loss phenomena and are considered important sources of interstellar dust. In this work, we employed a uniform method of spectral energy distribution fitting to analyze a large, and hence statistically signi...

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Bibliographic Details

Published in:	The Astrophysical Journal Supplement Series
Main Authors:	Jing Wen, Ming Yang, Jian Gao, Bingqiu Chen, Yi Ren, Biwei Jiang
Format:	Article
Language:	English
Published:	IOP Publishing 2024-01-01
Subjects:	Red supergiant stars Asymptotic giant branch stars Stellar mass loss Circumstellar dust Magellanic Clouds
Online Access:	https://doi.org/10.3847/1538-4365/ad7b33