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Journal articles
Kepler detected gravity-mode period spacings in a red giant star
P. G. Beck
1, *
T. R. Bedding
2
B. Mosser
3
D. Stello
2
R.A. Garcia
4
T. Kallinger
5
S. Hekker
6
Y. Elsworth
6
S. Frandsen
7
F. Carrier
1
J. de Ridder
1
C. Aerts
1
T. R. White
2
D. Huber
2
M.-A. Dupret
8
J. Montalbán
8
A. Miglio
8
A. Noels
8
W. J. Chaplin
6
H. Kjeldsen
9
J. Christensen-Dalsgaard
9
R. L. Gilliland
10
T. M. Brown
11
S. D. Kawaler
12
S. Mathur
13
J. M. Jenkins
14
*
Corresponding author
J. Christensen-Dalsgaard 9
Author
R. L. Gilliland 10
Author
T. M. Brown 11
Author
S. D. Kawaler 12
Author
S. Mathur 13
Author
J. M. Jenkins 14
Author
1
Instituut voor Sterrenkunde [Leuven] ( Celestijnenlaan 200D, 3001 Leuven - Belgium)
- KU Leuven - Catholic University of Leuven - Katholieke Universiteit Leuven (Oude Markt 13 - bus 5005, 3000 Leuven - Belgium)
2
SIfA - Sydney Institute for Astronomy (School of Physics, University of Sydney, NSW 2006, Australia - Australia)
- The University of Sydney (New South Wales 2006 - Australia)
3
LESIA (UMR_8109) - Laboratoire d'études spatiales et d'instrumentation en astrophysique (5, place Jules Janssen 92190 MEUDON - France)
- INSU - CNRS - Institut national des sciences de l'Univers : UMR8109 (INSU-CNRS 3 rue Michel-Ange, 75794 Paris Cedex 16 - France)
- Observatoire de Paris (61 Av de l'Observatoire 75014 PARIS - France)
- PSL - Université Paris sciences et lettres (60 rue Mazarine 75006 Paris - France)
- SU - Sorbonne Université (21 rue de l’École de médecine - 75006 Paris - France)
- CNRS - Centre National de la Recherche Scientifique : UMR8109 (France)
- UP - Université de Paris : UMR_8109 (85 boulevard Saint-Germain 75006 Paris - France)
4
AIM (UMR_7158 / UMR_E_9005 / UM_112) - Astrophysique Interprétation Modélisation (AIM - UMR 7158 - UMR E 9005,
ex "Astrophysique Interactions Multi-échelles",
Service d'astrophysique,
CEA/Saclay,
Orme des Merisiers
F-91191 GIF SUR YVETTE CEDEX - France)
- CEA - Commissariat à l'énergie atomique et aux énergies alternatives : UMR_E_9005 (Centre de Saclay Centre de Grenoble Centre de Cadarache etc - France)
- INSU - CNRS - Institut national des sciences de l'Univers (INSU-CNRS 3 rue Michel-Ange, 75794 Paris Cedex 16 - France)
- Université Paris-Saclay (Espace Technologique, Bat. Discovery - RD 128 - 2e ét., 91190 Saint-Aubin - France)
- CNRS - Centre National de la Recherche Scientifique : UMR_7158 (France)
- UP - Université de Paris : UMR_7158 (85 boulevard Saint-Germain 75006 Paris - France)
5
Department of Physics and Astronomy [Vancouver] (6224 Agricultural Road, Vancouver, BC V6T 1Z1 - Canada)
- UBC - University of British Columbia (Vancouver Campus, , 2329 West Mall, Vancouver, BC Canada V6T 1Z4 - Okanagan Campus, 3333 University Way, Kelowna, BC Canada V1V 1V7 - Canada)
6
School of Physics and Astronomy (United Kingdom)
- University of Birmingham [Birmingham] (Edgbaston Birmingham B15 2TT - United Kingdom)
7
AI PANNEKOEK - Astronomical Institute Anton Pannekoek (PO Box 94249, 1090 GE Amsterdam - Netherlands)
- UvA - University of Amsterdam [Amsterdam] (Spui 21 1012 WX Amsterdam - Netherlands)
8
Institut d'Astrophysique et de Géophysique [Liège] (17 Allée du 6 Août, B-4000 Liège - Belgium)
- Université de Liège (Place du 20-Août, 7 4000 Liège - Belgium)
9
Department of Physics and Astronomy [Aarhus] (Ny Munkegade 120, DK-8000 Aarhus C - Denmark)
- Aarhus University [Aarhus] (Nordre Ringgade 1 DK-8000 Aarhus C - Denmark)
10
STSci - Space Telescope Science Institute (3700 San Martin Drive, Baltimore, MD 21218, USA - United States)
11
Las Cumbres Observatory Global Telescope (Goleta, CA 93117, USA - United States)
12
Department of Physics and Astronomy [Ames, Iowa] (2323 Osborn Drive, Physics 0012, Ames, Iowa 50011-3160 - United States)
- ISU - Iowa State University ( Ames, Iowa 50011 - United States)
13
HAO - High Altitude Observatory (Boulder, CO 80307-3000 - United States)
- NCAR - National Center for Atmospheric Research [Boulder] (3090 Center Green Drive, Boulder, CO 80301 - United States)
14
SETI - Search for Extraterrestrial Intelligence Institute (Mountain View, CA 94043 - United States)
Abstract : Stellar interiors are inaccessible through direct observations. For this reason, helioseismologists made use of the Sun's acoustic oscillation modes to tune models of its structure. The quest to detect modes that probe the solar core has been ongoing for decades. We report the detection of mixed modes penetrating all the way to the core of an evolved star from 320 days of observations with the Kepler satellite. The period spacings of these mixed modes are directly dependent on the density gradient between the core region and the convective envelope
Document type :
Journal articles
Complete list of metadatas
https://hal-cea.archives-ouvertes.fr/cea-00863835
Contributor : Bruno Savelli <>
Submitted on : Tuesday, July 21, 2020 - 2:50:24 PM
Last modification on : Wednesday, September 23, 2020 - 4:40:16 AM
Contributor : Bruno Savelli <>
Submitted on : Tuesday, July 21, 2020 - 2:50:24 PM
Last modification on : Wednesday, September 23, 2020 - 4:40:16 AM
File
Kepbe4.pdf
Publication funded by an institution
Identifiers
- HAL Id : cea-00863835, version 1
- DOI : 10.1126/science.1201939
Collections
CEA | OBSPM | SORBONNE-UNIVERSITE | UP-SCIENCES | SU-SCIENCES | LESIA | CNRS | INSU | PSL
Citation
P. G. Beck, T. R. Bedding, B. Mosser, D. Stello, R.A. Garcia, et al.. Kepler detected gravity-mode period spacings in a red giant star. Science, American Association for the Advancement of Science, 2011, 332 (6026), pp.205. ⟨10.1126/science.1201939⟩. ⟨cea-00863835⟩
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