The CARMENES search for exoplanets around M dwarfs. Behaviour of the Paschen lines during flares and quiescence
The hydrogen Paschen lines are known activity indicators, but studies of them in M dwarfs during quiescence are as rare as their reports in flare studies. This situation is mostly caused by a lack of observations, owing to their location in the near-infrared regime, which is covered by few high-resolution spectrographs. We study the Paβ line, using
Fuhrmeister, B. et al.
Fecha de publicación:
10
2023