The orbital period of the optical/X-ray burster X 1735 - 444 (V926 Sco)

Details The orbital period of the optical/X-ray burster X 1735 - 444 (V926 Sco) The orbital period of the optical/X-ray burster X 1735 - 444 (V926 Sco)

Sep 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986mnras.222p..15c&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 222, Sept. 15, 1986, p. 15P-19P.

Astronomy and Astrophysics

Astronomy

23

Astronomical Photometry, Orbital Elements, Periodic Variations, Visible Spectrum, X Ray Sources, Charge Coupled Devices, Light Curve, Spectral Energy Distribution

Scientific paper

The authors present extensive CCD photometry of the optical counterpart
of X 1735-444 which reveals the orbital period of the system. It is
periodically variable with a period of 4.654 hr and a full amplitude of
0.15 mag. The mean modulation is quasi-sinusoidal; there are, however,
also significant intrinsic deviations from the mean light curve.

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