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1990ApJ...349..570L - Astrophys. J., 349, 570-579 (1990/January-3)
Line profile variations caused by low-frequency nonradial pulsations of rapidly rotating stars.
LEE U. and SAIO H.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): Line Profiles - Stars: Pulsation - Stars: Rotation
Simbad objects: 5
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