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Article Dans Une Revue Astronomical Notes / Astronomische Nachrichten Année : 2010

Asteroseismology of solar-type stars with Kepler I: Data analysis

1 School of Physics and Astronomy [Birmingham]
2 Department of Physics and Astronomy [Aarhus]
3 IAS - Institut d'astrophysique spatiale
4 AIM (UMR7158 / UMR_E_9005 / UM_112) - Astrophysique Interprétation Modélisation
5 Institute for Astronomy [Vienna]
6 SCD - Scientific Computing Division [Boulder]
7 Astronomical Institute [Wroclaw]
8 CAUP - Centro de Astrofísica da Universidade do Porto
9 DFA/FCUP - Departamento de Física e Astronomia [Porto]
10 SoMaS - School of Mathematics and Statistics [Sheffield]
11 STSci - Space Telescope Science Institute
12 Department of Astronomy [New Haven]
13 SIfA - Sydney Institute for Astronomy
14 Geneva Observatory
15 MERI - Materials and Engineering Research Institute [Sheffield]
16 HELIOS - LATMOS
17 LESIA - Laboratoire d'études spatiales et d'instrumentation en astrophysique
18 IAC - Instituto de Astrofisica de Canarias
19 Departamento de Astrofísica [La laguna]
20 AU - Astronomy Unit [London]
21 AGO - Département d'astrophysique, Géophysique et Océanographie
22 OAA - INAF - Osservatorio Astrofisico di Arcetri
23 Department of Astronomy and Physics [Halifax]
24 LANL - Los Alamos National Laboratory
25 Faculty of Mathematics [Vienna]
26 ZAH - Zentrum für Astronomie der Universität Heidelberg
27 Smithsonian Astrophysical Observatory
28 KIS - Kiepenheuer-Institut für Sonnenphysik
29 OHP - Observatoire de Haute-Provence
30 Astronomical Institute of Romanian Academy
31 JILA - Joint Institute for Laboratory Astrophysics
32 OACT - INAF - Osservatorio Astrofisico di Catania
33 Institute of Theoretical Astrophysics [Oslo]
34 NOT - Nordic Optical Telescope
Milena Martic
  • Fonction : Auteur
S. Mathur
K. Biazzo
S. Mathis
J. Schmitt

Résumé

We report on the first asteroseismic analysis of solar-type stars observed by Kepler. Observations of three G-type stars, made at one-minute cadence during the first 33.5 days of science operations, reveal high signal-to-noise solar-like oscillation spectra in all three stars: About 20 modes of oscillation can clearly be distinguished in each star. We discuss the appearance of the oscillation spectra, including the presence of a possible signature of faculae, and the presence of mixed modes in one of the three stars.
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Dates et versions

hal-00683333 , version 1 (18-10-2020)

Identifiants

Citer

C. Karoff, W.J. Chaplin, Thierry Appourchaux, Y. Elsworth, R.A. Garcia, et al.. Asteroseismology of solar-type stars with Kepler I: Data analysis. Astronomical Notes / Astronomische Nachrichten, 2010, 331 (9-10), pp.972-976. ⟨10.1002/asna.201011438⟩. ⟨hal-00683333⟩
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