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2016ApJ...829...68Y - Astrophys. J., 829, 68-68 (2016/October-1)
Estimating the radius of the convective core of main-sequence stars from observed oscillation frequencies.
YANG W.
Abstract (from CDS):
Abstract Copyright: © 2016. The American Astronomical Society. All rights reserved.
Journal keyword(s): convection - stars: evolution - stars: interiors - stars: oscillations , including pulsations - stars: oscillations , including pulsations
Simbad objects: 5
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