Observations of variable and transient X-ray sources with the Ariel V Sky Survey experiment

Astronomy and Astrophysics – Astronomy

Scientific paper

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Light Curve, Satellite Observation, Sky Surveys (Astronomy), Spaceborne Astronomy, X Ray Sources, Ariel Satellites, Binary Stars, Equatorial Orbits, Milky Way Galaxy, Stellar Models, Stellar Spectra, Stellar Winds, Uhuru Satellite, X Ray Stars

Scientific paper

Results obtained during the first six months in orbit of Ariel V with the Leicester Sky Survey are reviewed. Among 80 sources found by a scan of the Milky Way, 16 are new, and 11 Uhuru sources in the scanned region are not detected. Some of these sources may be transient. The light curve of Cen X-3 in a binary cycle shows a dip between phase 0.5 and 0.75, and a secondary maximum at the center of the dip. The dip and the maximum get progressively weaker in the succeeding cycles. These features are interpreted in terms of the stellar wind accretion model. Cyg X-1 observation for 14 days gives a broad minimum around superior conjunction. Four bright transient sources of nova-like light curves have been observed. The light curves and the spectra are given for TrA X-1 (A1524-62) and Tau X-T (A0535+26).

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