Magnetic field geometry of Alpha(2) Canum Venaticorum derived from circular-polarization profiles of metal lines

Details Magnetic field geometry of Alpha(2) Canum Venaticorum derived from circular-polarization profiles of metal lines Magnetic field geometry of Alpha(2) Canum Venaticorum derived from circular-polarization profiles of metal lines

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985pazh...11..371g&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 11, May 1985, p. 371-377) Soviet Astronomy Letters (ISSN 0360-0327), vol. 11, May-June

Astronomy and Astrophysics

Astronomy

4

A Stars, Circular Polarization, Line Spectra, Magnetic Field Configurations, Spectral Energy Distribution, Stellar Models, Iron, Stellar Magnetic Fields, Titanium

Scientific paper

Circular-polarization profiles of Fe II, Ti II lines are processed by solving the inverse problem to yield a model for the magnetic field geometry of the Ap star Alpha(2) CVn, allowing for the nonuniform distribution of elements over the stellar surface. The results are compared with other authors' models deduced by interpretation of effective-field curves.

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