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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Veröffentlicht in:	The Astrophysical journal 2024-11, Vol.975 (1), p.133
Hauptverfasser:	Liu, Shuai, Wei, Huigang, Shi, Jianrong, Li, Wenxian, Han, Henggeng, Liu, Jifeng, Yang, Shangbin
Format:	Artikel
Sprache:	eng
Schlagworte:	Calcium Extrasolar planets H alpha line High resolution Near infrared radiation Polar environments Polar regions Radiative transfer Spectra Spectrographs Stars Stellar activity Stellar atmospheres
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