Magnetic Doppler imaging of α2 Canum Venaticorum in all four Stokes parameters

Astronomy and Astrophysics

Volumn 513, Issue 2, 2010, Pages

  Kochukhov, O ^a   Wade, G A ^b  

^a UPPSALA UNIVERSITY   (Sweden)

^b ROYAL MILITARY COLLEGE OF CANADA   (Canada)

Author keywords

Polarization; Stars: atmospheres; Stars: chemically peculiar; Stars: individual: 2 CVn; Stars: magnetic field

Indexed keywords

CHEMICAL ELEMENTS; CHROMIUM; DOPPLER EFFECT; MAGNETIC FIELDS; NUMERICAL METHODS; POLARIZATION; STARS; TOPOLOGY;

ABUNDANCE DISTRIBUTION; CHEMICAL ABUNDANCE; CHEMICALLY PECULIAR-STARS; COMPLEX SURFACE; DOPPLER IMAGING; FIELD GEOMETRY; FIELD INTENSITY; FOUR STOKES PARAMETERS; HIGH CONTRAST; HIGH RESOLUTION; INHOMOGENEITIES; LINE PROFILES; LINEAR POLARIZATION; MAGNETIC FIELD MODELS; MAGNETIC FIELD TOPOLOGY; MAIN SEQUENCE STARS; NUMERICAL TECHNIQUES; OBSERVATIONAL METHOD; ROTATIONAL MODULATION; SPATIAL SCALE; SPECTROPOLARIMETERS; STARS: ATMOSPHERE; STARS: CHEMICALLY PECULIAR; STARS: MAGNETIC FIELD; STELLAR MAGNETIC FIELDS; SURFACE DISTRIBUTIONS; VECTOR MAPS;

MAGNETIC MATERIALS;

EID: 77952977549     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913860     Document Type: Article

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