Chromospheric Modeling of the Active M3V Star G 80–21 with RH1.5D

Chromospheric Modeling of the Active M3V Star G 80–21 with RH1.5D

This study investigates the active regions of the M3.0V star G 80–21 using the observed data from the CARMENES project with synthetic spectra generated by the RH1.5D radiative transfer code. The CARMENES project aims to search for exoplanets around M dwarfs using high-resolution near-infrared and op...

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Bibliographic Details
Main Authors: Shuai Liu, Huigang Wei, Jianrong Shi, Wenxian Li, Henggeng Han, Jifeng Liu, Shangbin Yang
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Stellar activity
Stellar atmospheres
Online Access:https://doi.org/10.3847/1538-4357/ad7f55

Internet

https://doi.org/10.3847/1538-4357/ad7f55

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