Solar-like oscillations in red giants observed with Kepler: Comparison of global oscillation parameters from different methods

被引：0

作者：

Hekker, S. ^{[1
]}

Elsworth, Y. ^{[1
]}

De Ridder, J. ^{[2
]}

Mosser, B. ^{[3
]}

García, R.A. ^{[4
]}

Kallinger, T. ^{[5
,6
]}

Mathur, S. ^{[7
]}

Huber, D. ^{[8
]}

Buzasi, D.L. ^{[9
]}

Preston, H.L. ^{[9
,10
]}

Hale, S.J. ^{[1
]}

Ballot, J. ^{[11
]}

Chaplin, W.J. ^{[1
]}

Régulo, C. ^{[12
,13
]}

Bedding, T.R. ^{[8
]}

Stello, D. ^{[8
]}

Borucki, W.J. ^{[14
]}

Koch, D.G. ^{[14
]}

Jenkins, J. ^{[15
]}

Allen, C. ^{[16
]}

Gilliland, R.L. ^{[17
]}

Kjeldsen, H. ^{[18
]}

Christensen-Dalsgaard, J. ^{[18
]}

机构：

[1] University of Birmingham, School of Physics and Astronomy, Edgbaston, Birmingham B15 2TT, United Kingdom

[2] Instituut voor Sterrenkunde, KU Leuven, Celestijnenlaan 200D, 3001 Leuven, Belgium

[3] LESIA, UMR8109, Université Pierre et Marie Curie, 92195 Meudon Cedex, France

[4] Laboratoire AIM, CEA/DSM-CNRS, Université Paris 7 Denis Diderot, 91191 Gif-sur-Yvette, France

[5] Department of Physics and Astronomy, University of British Colombia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada

[6] Institute for Astronomy, University of Vienna, Türkenschanzstrasse 17, 1180 Vienna, Austria

[7] High Altitude Observatory, NCAR, PO Box 3000, Boulder, CO 80307, United States

[8] Sydney Institute for Astronomy (SIfA), School of Physics, University of Sydney, NSW 2006, Australia

[9] Eureka Scientific, 2452 Delmer Street, Oakland, CA 94602-3017, United States

[10] Department of Mathematical Sciences, University of South Africa, Box 392, Unisa 0003, South Africa

[11] Laboratoire d'Astrophysique de Toulouse-Tarbes, Université de Toulouse, CNRS, 31400 Toulouse, France

[12] Universidad de la Laguna, Dpto de Astrofísica, 38206 Tenerife, Spain

[13] Instituto de Astrofísica de Canarias, 38205 La Laguna, Tenerife, Spain

[14] NASA Ames Research Center, MS 244-30, Moffet Field, CA 94035, United States

[15] SETI Institute, NASA Ames Research Center, MS 244-30, Moffet Field, CA 94035, United States

[16] Orbital Sciences Corp., NASA Ames Research Center, Moffet Field, CA 94035, United States

[17] Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, United States

[18] Department of Physics and Astronomy, Building 1520, Aarhus University, 8000 Aarhus C, Denmark

来源：

Astronomy and Astrophysics | 2010年 / 525卷 / 08期

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摘要：

引用

共 45 条

[21] Energetic Aspects of Non-Radial Solar-Like Oscillations in Red Giants
Dupret, Marc-Antoine
Belkacem, Kevin
RED GIANTS AS PROBES OF THE STRUCTURE AND EVOLUTION OF THE MILKY WAY, 2012, : 33 - 42
[22] Amplitudes of solar-like oscillations in red giants: Departures from the quasi-adiabatic approximation
Samadi, R.
Belkacem, K.
Dupret, M. -A.
Goupil, M. J.
Ludwig, H. -G.
Barban, C.
Baudin, F.
Caffau, E.
40TH LIEGE INTERNATIONAL ASTROPHYSICAL COLLOQUIUM AGEING LOW MASS STARS: FROM RED GIANTS TO WHITE DWARFS, 2013, 43
[23] MODELING KEPLER OBSERVATIONS OF SOLAR-LIKE OSCILLATIONS IN THE RED GIANT STAR HD 186355
Jiang, C.
Jiang, B. W.
Christensen-Dalsgaard, J.
Bedding, T. R.
Stello, D.
Huber, D.
Frandsen, S.
Kjeldsen, H.
Karoff, C.
Mosser, B.
Demarque, P.
Fanelli, M. N.
Kinemuchi, K.
Mullally, F.
ASTROPHYSICAL JOURNAL, 2011, 742 (02):
[24] Period-luminosity relations in evolved red giants explained by solar-like oscillations
Mosser, B.
Dziembowski, W. A.
Belkacem, K.
Goupil, M. J.
Michel, E.
Samadi, R.
Soszynski, I.
Vrard, M.
Elsworth, Y.
Hekker, S.
Mathur, S.
ASTRONOMY & ASTROPHYSICS, 2013, 559
[25] Period-luminosity relations in evolved red giants explained by solar-like oscillations
Mosser, B.
Dziembowski, W.A.
Belkacem, K.
Goupil, M.J.
Michel, E.
Samadi, R.
Soszyński, I.
Vrard, M.
Elsworth, Y.
Hekker, S.
Mathur, S.
Astronomy and Astrophysics Review, 2013, 559
[26] Theoretical amplitudes and lifetimes of non-radial solar-like oscillations in red giants
Dupret, M. -A.
Belkacem, K.
Samadi, R.
Montalban, J.
Moreira, O.
Miglio, A.
Godart, M.
Ventura, P.
Ludwig, H. -G.
Grigahcene, A.
Goupil, M. -J.
Noels, A.
Caffau, E.
ASTRONOMY & ASTROPHYSICS, 2009, 506 (01) : 57 - 67
[27] Period-luminosity relations in evolved red giants explained by solar-like oscillations
1600, EDP Sciences (559):
[28] ASTEROSEISMOLOGY OF RED GIANTS FROM THE FIRST FOUR MONTHS OF KEPLER DATA: GLOBAL OSCILLATION PARAMETERS FOR 800 STARS
Huber, D.
Bedding, T. R.
Stello, D.
Mosser, B.
Mathur, S.
Kallinger, T.
Hekker, S.
Elsworth, Y. P.
Buzasi, D. L.
De Ridder, J.
Gilliland, R. L.
Kjeldsen, H.
Chaplin, W. J.
Garcia, R. A.
Hale, S. J.
Preston, H. L.
White, T. R.
Borucki, W. J.
Christensen-Dalsgaard, J.
Clarke, B. D.
Jenkins, J. M.
Koch, D.
ASTROPHYSICAL JOURNAL, 2010, 723 (02): : 1607 - 1617
[29] Asteroseismology of 16,000 Kepler Red Giants: Global Oscillation Parameters, Masses, and Radii
Yu, Jie
Huber, Daniel
Bedding, Timothy R.
Stello, Dennis
Hon, Marc
Murphy, Simon J.
Khanna, Shourya
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2018, 236 (02):
[30] Magnetic activity of red giants: Correlation between the amplitude of solar-like oscillations and chromospheric indicators
Gehan, C.
Godoy-Rivera, D.
Gaulme, P.
ASTRONOMY & ASTROPHYSICS, 2024, 686

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