EK Eridani: The tip of the iceberg of giants which have evolved from magnetic Ap stars

Astronomy and Astrophysics

Volumn 491, Issue 2, 2008, Pages 499-505

  Auriere M ^a   Konstantinova Antova, R ^b   Petit, P ^a   Charbonnel, C ^a,c   Dintrans, B ^a   Lignieres F ^a   Roudier, T ^a   Alecian, E ^d   Donati, J F ^a   Landstreet, J D ^e   Wade, G A ^d  

^a UNIVERSITÉ DE TOULOUSE   (France)

^b INSTITUTE OF ASTRONOMY   (Bulgaria)

^c UNIVERSITÉ DE GENÈVE   (Switzerland)

^d ROYAL MILITARY COLLEGE OF CANADA   (Canada)

^e UNIVERSITY OF WESTERN ONTARIO   (Canada)

Author keywords

Stars: individual: EK Eridani; Stars: late type; Stars: magnetic fields

Indexed keywords

CALCIUM; CURVE FITTING; FADING (RADIO); MAGNETIC FIELD MEASUREMENT; MAGNETIC FIELDS; MAGNETIC MATERIALS; ROTATION; SIGNAL TO NOISE RATIO; STARS;

DECONVOLUTION METHODS; LEAST SQUARES; LONGITUDINAL MAGNETIC FIELDS; POLOIDAL COMPONENTS; RED GIANTS; SIGNAL-TO-NOISE RATIOS; SPECTROPOLARIMETER; STARS: INDIVIDUAL: EK ERIDANI; STARS: MAGNETIC FIELDS; SURFACE MAGNETIC FIELDS;

MAGNETISM;

EID: 57049155589     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200810502     Document Type: Article

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