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1999A&AS..135..383M - Astron. Astrophys., Suppl. Ser., 135, 383-390 (1999/March-1)
An improved method for the determination of the orbital parameters of a binary system that contains a pulsating component.
MOLENBERGHS G., AERTS C. and DE CAT P.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): methods: statistical - stars: oscillations - binaries: spectroscopic
Simbad objects: 12
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