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A Seismic and Gravitationally Bound Double Star Observed by Kepler Implication for the Presence of a Convective Core

AuthID
P-00S-5DT

Author(s)

Appourchaux, T

Antia, HM

Ball, W

Creevey, O

Lebreton, Y

Verma, K

Vorontsov, S

Campante, TL

Davies, GR

Gaulme, P

[+1]·

Horch, E

Howell, S

Everett, M

Ciardi, D

Fossati, L

Miglio, A

Montalban, J

Chaplin, WJ

Garcia, RA

Gizon, L

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Document Type

Article

Year published

2015

Published

in ASTRONOMY & ASTROPHYSICS, ISSN: 1432-0746

Volume: 582

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Publication Identifiers

DOI: 10.1051/0004-6361/201526610

Scopus: 2-s2.0-84942741254

Wos: WOS:000363538500025

Source Identifiers

ISSN: 1432-0746

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All authors

Name Order	Nome	Name Order	Nome	Name Order	Nome
1	Appourchaux, T;	2	Antia, HM;	3	Ball, W;
4	Creevey, O;	5	Lebreton, Y;	6	Verma, K;
7	Vorontsov, S;	8	Campante, TL ;	9	Davies, GR;
10	Gaulme, P;	11	Regulo, C;	12	Horch, E;
13	Howell, S;	14	Everett, M;	15	Ciardi, D;
16	Fossati, L;	17	Miglio, A;	18	Montalban, J;
19	Chaplin, WJ;	20	Garcia, RA;	21	Gizon, L;

A Seismic and Gravitationally Bound Double Star Observed by Kepler Implication for the Presence of a Convective Core

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A Seismic and Gravitationally Bound Double Star Observed by Kepler Implication for the Presence of a Convective Core

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