Very regular high-frequency pulsation modes in young intermediate-mass stars

Asteroseismology probes the internal structures of stars by using their natural pulsation frequencies1. It relies on identifying sequences of pulsation modes that can be compared with theoretical models, which has been done successfully for many classes of pulsators, including low-mass solar-type st...

Ausführliche Beschreibung

Bibliographische Detailangaben

Veröffentlicht in:	NATURE 2020-05, Vol.581 (7807), p.147-+
Hauptverfasser:	Bedding, Timothy R, Murphy, Simon J, Hey, Daniel R, Huber, Daniel, Li, Tanda, Smalley, Barry, Stello, Dennis, White, Timothy R, Ball, Warrick H, Chaplin, William J, Colman, Isabel L, Fuller, Jim, Gaidos, Eric, Harbeck, Daniel R, Hermes, J.J, Holdsworth, Daniel L, Li, Gang, Li, Yaguang, Mann, Andrew W, Reese, Daniel R, Sekaran, Sanjay, Yu, Jie, Antoci, Victoria, Bergmann, Christoph, Brown, Timothy M, Howard, Andrew W, Ireland, Michael J, Isaacson, Howard, Jenkins, Jon M, Kjeldsen, Hans, McCully, Curtis, Rabus, Markus, Rains, Adam D, Ricker, George R, Tinney, Christopher G, Vanderspek, Roland K
Format:	Artikel
Sprache:	eng
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!