Open AccessThe orbital period of the optical/X-ray burster X1735-444 (V926 Sco)
Author(s) -
R. H. D. Corbet,
J. R. Thorstensen,
P. A. Charles,
J. W. Menzies,
T. Naylor,
A. P. Smale
Publication year - 1986
Publication title -
monthly notices of the royal astronomical society
Language(s) - French
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-2966
pISSN - 0035-8711
DOI - 10.1093/mnras/222.1.15p
Subject(s) - physics , photometry (optics) , light curve , orbital period , amplitude , astrophysics , astronomy , variable star , period (music) , optics , stars , acoustics
Photometrie CCD de l'associe optique de X 1735-444, revelant la periode orbitale du systeme. Il varie periodiquement avec une periode de 4,654 h et une amplitude totale de 0,15 mag. La modulation moyenne est quasi sinusoidale
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