Magnetic field structure in single late-type giants: The effectively single giant V390 Aurigae

Astronomy and Astrophysics

Volumn 541, Issue , 2012, Pages

  Konstantinova Antova, R ^a,b   Auriere M ^b   Petit, P ^b   Charbonnel, C ^b,c   Tsvetkova, S ^a   Lebre A ^d   Bogdanovski, R ^a  

^a INSTITUTE OF ASTRONOMY   (Bulgaria)

^b UNIVERSITÉ DE TOULOUSE   (France)

^c UNIVERSITÉ DE GENÈVE   (Switzerland)

^d UNIV MONTPELLIER   (France)

Author keywords

Dynamo; Magnetic fields; Stars: individual: V390 Aur

Indexed keywords

AZIMUTHAL FIELD; DATA SETS; DOPPLER IMAGING; FIELD STRUCTURES; FUNDAMENTAL PARAMETERS; HIGH LATITUDES; INVERSION METHODS; LATE-TYPE; LEAST SQUARE; LONGITUDINAL COMPONENTS; MAGNETIC-FIELD GEOMETRY; METALLICITIES; MODEL ATMOSPHERE; POSITIVE POLARITY; RADIAL MAGNETIC FIELD; ROSSBY NUMBERS; ROTATION PROPERTY; SIMULTANEOUS MEASUREMENT; SPECTROPOLARIMETERS; SPECTROPOLARIMETRY; STARS: INDIVIDUAL; STELLAR MODELS; STELLAR STRUCTURE; TOROIDAL FIELDS; WAVELENGTH RANGES;

DC GENERATORS; DYES; ELECTRIC GENERATORS; INTERACTIVE DEVICES; STARS;

MAGNETIC FIELDS;

EID: 84860309377     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201116690     Document Type: Article

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