The first evidence for multiple pulsation axes: A new rapidly oscillating Ap star in the Kepler field, KIC10195926

Monthly Notices of the Royal Astronomical Society

Volumn 414, Issue 3, 2011, Pages 2550-2566

  Kurtz, D W ^a   Cunha, M S ^b   Saio, H ^c   Bigot, L ^d   Balona, L A ^e   Elkin, V G ^a   Shibahashi, H ^f   Brandao I M ^b   Uytterhoeven, K ^g   Frandsen, S ^h   Frimann, S ^h,i   Hatzes, A ^j   Lueftinger, T ^k   Gruberbauer, M ^l   Kjeldsen, H ^h   Christensen Dalsgaard, J ^h   Kawaler, S D ^m  

^a UNIVERSITY OF CENTRAL LANCASHIRE   (United Kingdom)

^b CENTRO DE ASTROFÍSICA   (Portugal)

^c TOHOKU UNIVERSITY   (Japan)

^d UNIVERSITÉ CÔTE D'AZUR   (France)

^e SOUTH AFRICAN ASTRONOMICAL OBSERVATORY   (South Africa)

^f UNIVERSITY OF TOKYO   (Japan)

^g CEA SACLAY   (France)

^h AARHUS UNIVERSITY   (Denmark)

ⁱ NORDIC OPTICAL TELESCOPE   (Spain)

^j THÜRINGER LANDESSTERNWARTE TAUTENBURG   (Germany)

^k Institut fur Astronomie Vienna   (Austria)

^l SAINT MARY S UNIVERSITY   (Canada)

^m IOWA STATE UNIVERSITY   (United States)

more..

Author keywords

Stars: chemically peculiar; Stars: individual: KIC10195926; Stars: magnetic field; Stars: oscillations; Starspots

Indexed keywords

MAGNETISM; SEPARATION; STARS;

DIPOLE MODE; PULSATION MODES; STAR OSCILLATIONS; STAR: INDIVIDUAL: KIC10195926; STARS: BE; STARS: CHEMICALLY PECULIAR; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS: MAGNETIC FIELD; STARSPOTS; SUBHARMONICS;

RARE EARTHS;

EID: 79959444742     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2011.18572.x     Document Type: Article

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