Radius determination of solar-type stars using asteroseismology: What to expect from the kepler mission

Astrophysical Journal

Volumn 700, Issue 2, 2009, Pages 1589-1602

  Stello, Dennis ^a,b   Chaplin, William J ^c   Bruntt, Hans ^a   Creevey, Orlagh L ^d   García Hernndez, Antonio ^e   Monteiro, Mario J P F G ^f,g   Moya, Andrés ^e   Quirion, Pierre Olivier ^b   Sousa, Sergio G ^f,g   Surez, Juan Carlos ^e   Appourchaux, Thierry ^h   Arentoft, Torben ^b   Ballot, Jerome ^i,j   Bedding, Timothy R ^a   Christensen Dalsgaard, Jørgen ^b   Elsworth, Yvonne ^c   Fletcher, Stephen T ^k   García, Rafael A ^l   Houdek, Günter ^m,n   Jiménez Reyes, Sebastian J ^d   Kjeldsen, Hans ^b   New, Roger ^j   Régulo, Clara ^d,o   Salabert, David ^d,p   Toutain, Thierry ^c   more..

^a UNIVERSITY OF SYDNEY   (Australia)

^b AARHUS UNIVERSITY   (Denmark)

^c UNIVERSITY OF BIRMINGHAM   (United Kingdom)

^d INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^e INSTITUTO DE ASTROFÍSICA DE ANDALUCÍA CSIC   (Spain)

^f CENTRO DE ASTROFÍSICA   (Portugal)

^g UNIVERSITY OF PORTO   (Portugal)

^h UNIVERSITÉ PARIS SUD   (France)

ⁱ MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^j UNIVERSITÉ DE TOULOUSE   (France)

^k SHEFFIELD HALLAM UNIVERSITY   (United Kingdom)

^l CEA SACLAY   (France)

^m UNIVERSITY OF VIENNA   (Austria)

ⁿ UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^o UNIVERSIDAD DE LA LAGUNA   (Spain)

^p NATIONAL SOLAR OBSERVATORY   (United States)

more..

Author keywords

Stars: fundamental parameters; Stars: interiors; Stars: oscillations

Indexed keywords

EID: 70549096272     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/700/2/1589     Document Type: Article

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