Analytical Calculation of Stokes Profiles of Rotating Stellar Magnetic Dipole
The observation of the polarization emerging from a rotating star at different phases opens up the possibility to map the magnetic field in the stellar surface thanks to the well-known Zeeman-Doppler imaging. When the magnetic field is sufficiently weak, the circular and linear polarization profiles locally in each point of the star are
Martínez-González, M. J. et al.
Fecha de publicación:
8
2012