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1996A&A...309..775S - Astronomy and Astrophysics, volume 309775-776 (1996/5-3)
Possible change of the orbital period of the nova-like binary V Sagittae.
SIMON V.
Abstract (from CDS):
Analysis of the available minimum timings of this cataclysmic binary spanning 31 years revealed fairly stable orbital period. The parabolic course leads to very small {DELTA}P/P=-2.94x10–10.
Abstract Copyright: ∼
Journal keyword(s): binaries: eclipsing - circumstellar matter - novae, cataclysmic variables - stars: individual: V Sge
Simbad objects: 1
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