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Infrared Properties of Carbon Stars in Our Galaxy
DOI: 10.3847/1538-4365/ad38b5 Bibcode: 2024ApJS..272...16S

Suh, Kyung-Won

We explore the characteristics of carbon stars within our Galaxy through a comprehensive analysis of observational data spanning visual and infrared (IR) bands. Leveraging data sets from IRAS, the Infrared Space Observatory, Akari, the Midcourse Space Experiment, the Two Micron All Sky Survey, the Wide-field Infrared Survey Explorer (WISE), Gaia D…

2024 The Astrophysical Journal Supplement Series
ISO AKARI Gaia 2
Mass-loss Rate of Highly Evolved Stars in the Magellanic Clouds
DOI: 10.3847/1538-4365/ad7b33 Bibcode: 2024ApJS..275...33W

Yang, Ming; Gao, Jian; Ren, Yi +3 more

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 significant, sample of approximately 40,000 RSGs and A…

2024 The Astrophysical Journal Supplement Series
Herschel AKARI Gaia 1