Zeeman-Doppler imaging of active stars. I - Basic principles

Details Zeeman-Doppler imaging of active stars. I - Basic principles Zeeman-Doppler imaging of active stars. I - Basic principles

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...225..456s&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 225, no. 2, Nov. 1989, p. 456-466.

Statistics

Computation

125

Computational Astrophysics, Doppler Effect, Stellar Activity, Stellar Spectra, Zeeman Effect, Fourier Transformation, Integral Equations, Magnetic Field Configurations, Polarimetry, Stellar Rotation

Scientific paper

Methods are proposed for the analysis of polarimetric measurements in the spectra of active stars. The Doppler effect of rapidly rotating stars may help to disclose magnetic field distributions, which otherwise may not be seen due to even distribution of positive and negative fields. The methods developed allow one to average the measurements of many lines.

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