Optical variability of the low-mass, X-ray binary 1556-605

Details Optical variability of the low-mass, X-ray binary 1556-605 Optical variability of the low-mass, X-ray binary 1556-605

Feb 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990pasp..102..144s&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 102, Feb. 1990, p. 144-147.

Astronomy and Astrophysics

Astronomy

3

Stellar Mass, Stellar Spectrophotometry, X Ray Binaries, Charge Coupled Devices, Exosat Satellite, Light Curve, Stellar Orbits

Scientific paper

BVRI photometry of the low-mass, X-ray binary 1556-605, obtained during
five nights in June 1988, failed to identify an underlying orbital
period. Nightly variations of 0.3 magnitude in V were present, but the
colors of the system remained constant.

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