PULSATING B-TYPE STARS IN THE OPEN CLUSTER NGC 884: FREQUENCIES, MODE IDENTIFICATION, AND ASTEROSEISMOLOGY

Recent progress in the seismic interpretation of field beta Cep stars has resulted in improvements of the physical description in the stellar structure and evolution model computations of massive stars. Further asteroseismic constraints can be obtained from studying ensembles of stars in a young ope...

Ausführliche Beschreibung

Gespeichert in:

Bibliographische Detailangaben
Veröffentlicht in:	The Astronomical journal 2013-10, Vol.146 (4), p.1-17
Hauptverfasser:	Saesen, S, Briquet, M, Aerts, C, Miglio, A, Carrier, F
Format:	Artikel
Sprache:	eng
Schlagworte:	Age ASTRONOMY ASTROPHYSICS ASTROPHYSICS, COSMOLOGY AND ASTRONOMY Aérospatiale, astronomie & astrophysique CALCULATION METHODS CHEMICAL COMPOSITION Clusters COMPARATIVE EVALUATIONS DIPOLES Estimates FREQUENCY ANALYSIS LIMITING VALUES Massive stars Mathematical models Open clusters open clusters and associations: individual: NGC 884 OSCILLATIONS PERIODICITY Physical, chemical, mathematical & earth Sciences Physique, chimie, mathématiques & sciences de la terre Space science, astronomy & astrophysics STAR CLUSTERS STAR EVOLUTION STAR MODELS STARS stars: early-type stars: oscillations Stellar structure techniques: photometric
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!

Schreiben Sie den ersten Kommentar!