Magnetic Fields in M-dwarf Members of the Pleiades Open Cluster Using APOGEE Spectra
Average magnetic field measurements are presented for 62 M-dwarf members of the Pleiades open cluster, derived from Zeeman-enhanced Fe I lines in the H band. A Markov Chain Monte Carlo methodology was employed to model magnetic filling factors using Sloan Digital Sky Survey (SDSS) IV APOGEE high-resolution spectra, along with the radiative transfer
Wanderley, Fábio et al.
Fecha de publicación:
8
2024