Asteroseismic inferences on red giants in open clusters NGC 6791, NGC 6819, and NGC 6811 using Kepler

Astronomy and Astrophysics

Volumn 530, Issue , 2011, Pages

  Hekker, S ^a,b   Basu, S ^c   Stello, D ^d   Kallinger, T ^e   Grundahl, F ^f   Mathur, S ^g   Garcia R A ^h   Mosser, B ⁱ   Huber, D ^d   Bedding, T R ^d   Szabo R ^j   De Ridder, J ^k   Chaplin, W J ^b   Elsworth, Y ^b   Hale, S J ^b   Christensen Dalsgaard, J ^f   Gilliland, R L ^l   Still, M ^m   McCauliff, S ^m   Quintana, E V ^m  

^a UNIVERSITY OF AMSTERDAM   (Netherlands)

^b UNIVERSITY OF BIRMINGHAM   (United Kingdom)

^c YALE UNIVERSITY   (United States)

^d UNIVERSITY OF SYDNEY   (Australia)

^e UNIVERSITY OF BRITISH COLUMBIA   (Canada)

^f AARHUS UNIVERSITY   (Denmark)

^g NATIONAL CENTER FOR ATMOSPHERIC RESEARCH   (United States)

^h UNIVERSITÉ PARIS DIDEROT   (France)

ⁱ UNIVERSITÉ PARIS DIDEROT   (France)

^j KONKOLY OBSERVATORY   (Hungary)

^k KU LEUVEN   (Belgium)

^l STScI   (United States)

^m NASA AMES RESEARCH CENTER   (United States)

more..

Author keywords

Asteroseismology; Methods: observational; Open clusters and associations: general; Stars: late type; Techniques: photometric

Indexed keywords

ASTEROSEISMOLOGY; METHODS: OBSERVATIONAL; OPEN CLUSTERS AND ASSOCIATIONS: GENERAL; STARS: LATE-TYPE; TECHNIQUES: PHOTOMETRIC;

ASTROPHYSICS; TEMPERATURE;

STARS;

EID: 79956115938     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201016303     Document Type: Article

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