The Aarhus red giants challenge

Contact. The large quantity of high-quality asteroseismic data that have been obtained from space-based photometric missions and the accuracy of the resulting frequencies motivate a careful consideration of the accuracy of computed oscillation frequencies of stellar models, when applied as diagnosti...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2020-03, Vol.635
Hauptverfasser:	Christensen-Dalsgaard, J, V. Silva Aguirre, Cassisi, S, M. Miller Bertolami, 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
Format:	Artikel
Sprache:	eng
Schlagworte:	Accuracy Astronomical models Computation Properties (attributes) Red giant stars Stellar evolution Stellar interiors Stellar models Stellar oscillations Stellar seismology
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