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Publikováno v:
Astronomy & Astrophysics. 670:L16
Despite their importance in stellar evolution, little is known about magnetic fields in the interior of stars. The recent seismic detection of magnetic fields in the core of several red giant stars has given measurements of their strength and informa
Autor:
Tiago L. Campante, M. L. Winther, M. T. Clara, Mário J. P. F. G. Monteiro, K. Belkacem, Kuldeep Verma, M. S. Cunha, Anthony Noll, V. Aguirre Børsen-Koch, Sarbani Basu, William J. Chaplin, Warrick H. Ball, Amalie Stokholm, Daniel R. Reese, J. L. Rørsted, Ian W. Roxburgh, Marie-Jo Goupil, Benard Nsamba, R. M. Ouazzani, S. Deheuvels, Joel J. M. Ong, Joergen Christensen-Dalsgaard
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, ⟨10.1093/mnras/stab2886⟩
Cunha, M S, Roxburgh, I W, Børsen-Koch, V A, Ball, W H, Basu, S, Chaplin, W J, Goupil, M-J, Nsamba, B, Ong, J J M, Reese, D R, Verma, K, Belkacem, K, Campante, T, Christensen-Dalsgaard, J, Clara, M T, Deheuvels, S, Monteiro, M J P F G, Noll, A, Ouazzani, R-M, Mosumgaard, J R, Stokholm, A & Winther, M L 2021, ' PLATO hare-and-hounds exercise : asteroseismic model fitting of main-sequence solar-like pulsators ', Monthly Notices of the Royal Astronomical Society, vol. 508, no. 4, pp. 5864-5885 . https://doi.org/10.1093/mnras/stab2886
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, ⟨10.1093/mnras/stab2886⟩
Cunha, M S, Roxburgh, I W, Børsen-Koch, V A, Ball, W H, Basu, S, Chaplin, W J, Goupil, M-J, Nsamba, B, Ong, J J M, Reese, D R, Verma, K, Belkacem, K, Campante, T, Christensen-Dalsgaard, J, Clara, M T, Deheuvels, S, Monteiro, M J P F G, Noll, A, Ouazzani, R-M, Mosumgaard, J R, Stokholm, A & Winther, M L 2021, ' PLATO hare-and-hounds exercise : asteroseismic model fitting of main-sequence solar-like pulsators ', Monthly Notices of the Royal Astronomical Society, vol. 508, no. 4, pp. 5864-5885 . https://doi.org/10.1093/mnras/stab2886
Asteroseismology is a powerful tool to infer fundamental stellar properties. The use of these asteroseismic-inferred properties in a growing number of astrophysical contexts makes it vital to understand their accuracy. Consequently, we performed a ha
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::79360c195d78ab7dbcd15d32a6d286a2
https://hal.archives-ouvertes.fr/hal-03404552
https://hal.archives-ouvertes.fr/hal-03404552
Akademický článek
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Autor:
T. Lopez, Isabelle Boisse, S. Deheuvels, Zahra Essack, David Baker, F. Debras, P. C. König, T. Forveille, J. Villasenor, Sergio Hoyer, X. Delfosse, Keivan G. Stassun, Patricia T. Boyd, Nuno C. Santos, George R. Ricker, Guillaume Hébrard, Olivier Demangeon, C. Moutou, H. P. Osborn, C. Ziegler, P. Guerra, D. Laloum, S. C. C. Barros, Michael Vezie, R. Vanderspek, X. Bonfils, Flavien Kiefer, Joshua N. Winn, Katharine Hesse, D. W. Latham, S. Dalal, Magali Deleuil, Sara Seager, Jose-Manuel Almenara, P. Cortés-Zuleta, E. Girardin, Eder Martioli, Jon M. Jenkins, Paul Benni, Allyson Bieryla, Karen A. Collins, N. Heidari, Bill Wohler
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 653, pp.A147. ⟨10.1051/0004-6361/202141151⟩
Astronomy and Astrophysics-A&A, 2021, 653, pp.A147. ⟨10.1051/0004-6361/202141151⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 653, pp.A147. ⟨10.1051/0004-6361/202141151⟩
Astronomy and Astrophysics-A&A, 2021, 653, pp.A147. ⟨10.1051/0004-6361/202141151⟩
We present the discovery of two new transiting extrasolar planet candidates identified as TOI-1296.01 and TOI-1298.01 by the Transiting Exoplanet Survey Satellite (TESS). The planetary nature of these candidates has been secured with the SOPHIE high-
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::20d4477ada34eb8c105191801354054e
Autor:
Maurizio Salaris, V. Silva Aguirre, Santi Cassisi, Anwesh Mazumdar, Dennis Stello, George C. Angelou, Andrea Miglio, R. M. Ouazzani, Federico Spada, Earl P. Bellinger, Diego Bossini, Tiara Battich, M. M. Miller Bertolami, Jakob Rørsted Mosumgaard, Richard H. D. Townsend, K. B. Nielsen, Adriano Pietrinferni, Chen Jiang, S. Deheuvels, Saskia Hekker, A. Weiss, Jørgen Christensen-Dalsgaard, Aldo Serenelli, T. Constantino, Patrick Eggenberger, Yveline Lebreton
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2020, 635, pp.A165. ⟨10.1051/0004-6361/201935843⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Silva Aguirre, V, Christensen-Dalsgaard, J, Cassisi, S, Miller Bertolami, M, Serenelli, A, Stello, D, Weiss, A, Angelou, G, Jiang, C, Lebreton, Y, Spada, F, Bellinger, E P, Deheuvels, S, Ouazzani, R M, Pietrinferni, A, Mosumgaard, J R, Townsend, R H D, Battich, T, Bossini, D, Constantino, T, Eggenberger, P, Hekker, S, Mazumdar, A, Miglio, A, Nielsen, K B & Salaris, M 2020, ' The Aarhus red giants challenge. I. Stellar structures in the red giant branch phase ', Astronomy & Astrophysics, vol. 635, A164 . https://doi.org/10.1051/0004-6361/201935843
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 635, pp.A165. ⟨10.1051/0004-6361/201935843⟩
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Astronomy and Astrophysics-A&A, 2020, 635, pp.A165. ⟨10.1051/0004-6361/201935843⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Silva Aguirre, V, Christensen-Dalsgaard, J, Cassisi, S, Miller Bertolami, M, Serenelli, A, Stello, D, Weiss, A, Angelou, G, Jiang, C, Lebreton, Y, Spada, F, Bellinger, E P, Deheuvels, S, Ouazzani, R M, Pietrinferni, A, Mosumgaard, J R, Townsend, R H D, Battich, T, Bossini, D, Constantino, T, Eggenberger, P, Hekker, S, Mazumdar, A, Miglio, A, Nielsen, K B & Salaris, M 2020, ' The Aarhus red giants challenge. I. Stellar structures in the red giant branch phase ', Astronomy & Astrophysics, vol. 635, A164 . https://doi.org/10.1051/0004-6361/201935843
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 635, pp.A165. ⟨10.1051/0004-6361/201935843⟩
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
[Context] With the advent of space-based asteroseismology, determining accurate properties of red-giant stars using their observed oscillations has become the focus of many investigations due to their implications in a variety of fields in astrophysi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::32ca00bc11201ce0701dca512053533b
https://hal.science/hal-02523040/file/aa35843-19.pdf
https://hal.science/hal-02523040/file/aa35843-19.pdf
Context: The internal characteristics of stars, such as their core rotation rates, are obtained via asteroseismic observations. A comparison of core rotation rates found in this way with core rotation rates as predicted by stellar evolution models de
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5cb2d64c2b8ac3024244f5e5f0d008d8