Solar-like oscillations from the depths of the red-giant star KIC4351319 observed with Kepler

Monthly Notices of the Royal Astronomical Society

Volumn 415, Issue 4, 2011, Pages 3783-3797

  di Mauro, M P ^a   Cardini, D ^a   Catanzaro, G ^b   Ventura, R ^b   Barban, C ^c   Bedding, T R ^d   Christensen Dalsgaard, J ^e   de Ridder, J ^f   Hekker, S ^g,h   Huber, D ^d   Kallinger, T ^i,j   Miglio, A ^g,k   Montalban, J ^k   Mosser, B ^c   Stello, D ^d   Uytterhoeven, K ^l,m   Kinemuchi, K ⁿ   Kjeldsen, H ^e   Mullally, F ⁿ   Still, M ⁿ  

^a INAF IASF ROMA   (Italy)

^b INAF OSSERVATORIO ASTROFISICO DI CATANIA   (Italy)

^c UNIVERSITÉ PARIS DIDEROT   (France)

^d UNIVERSITY OF SYDNEY   (Australia)

^e AARHUS UNIVERSITY   (Denmark)

^f UNIVERSITY OF LEUVEN   (Belgium)

^g UNIVERSITY OF BIRMINGHAM   (United Kingdom)

^h UNIVERSITY OF AMSTERDAM   (Netherlands)

ⁱ UNIVERSITY OF BRITISH COLUMBIA   (Canada)

^j UNIVERSITY OF VIENNA   (Austria)

^k UNIVERSITY OF LIÈGE   (Belgium)

^l CEA SACLAY   (France)

^m KIEPENHEUER INSTITUT FÜR SONNENPHYSIK   (Germany)

ⁿ NASA AMES RESEARCH CENTER   (United States)

more..

Author keywords

Stars: AGB and post AGB; Stars: evolution; Stars: fundamental parameters; Stars: individual: KIC 4351319; Stars: oscillations; Stars: solar type

Indexed keywords

GIANT STARS;

OSCILLATION FREQUENCY; P MODES; P-MODES; STAR OSCILLATIONS; STAR: EVOLUTION; STAR: INDIVIDUAL: KIC 4351319; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS: SOLAR TYPES; STARS:AGB AND POST AGB; STARS:FUNDAMENTAL PARAMETERS;

SIGNAL TO NOISE RATIO;

EID: 80051805362     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2011.18996.x     Document Type: Article

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