14 Ceti: A probable Ap-star-descendant entering the Hertzsprung gap

Astronomy and Astrophysics

Volumn 543, Issue , 2012, Pages

  Auriere M ^a   Konstantinova Antova, R ^a,b   Petit, P ^a   Charbonnel, C ^a,c   Van Eck, S ^d   Donati, J F ^a   Lignieres F ^a   Roudier, T ^a  

^a IRAP   (France)

^b INSTITUTE OF ASTRONOMY   (Bulgaria)

^c UNIVERSITÉ DE GENÈVE   (Switzerland)

^d UNIVERSITÉ LIBRE DE BRUXELLES   (Belgium)

Author keywords

Stars: individual: 14 Ceti; Stars: late type; Stars: magnetic field

Indexed keywords

DECONVOLUTION METHOD; EMISSION CORE; HIGH SIGNAL-TO-NOISE RATIO; LEAST SQUARE; LONG-TERM TREND; LONGITUDINAL MAGNETIC FIELDS; MAGNETIC ACTIVITY; PRE-MAIN-SEQUENCE; RADIAL VELOCITY; SPECTRAL CLASS; SPECTROPOLARIMETERS; STARS: INDIVIDUAL; STARS: MAGNETIC FIELD; STARS:LATE TYPE; SURFACE MAGNETIC FIELD; TIME-SCALES; X-RAY EMISSION;

FADING (RADIO); LEAST SQUARES APPROXIMATIONS; MAGNETIC FIELDS;

STARS;

EID: 84863668689     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201219324     Document Type: Article

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