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Optical photometry of the eclipsing Large Magellanic Cloud supersoft source CAL 87

Monthly Notices of the Royal Astronomical Society(1997)

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Abstract
We present optical photometry of the eclipsing supersoft source CAL 87. These observations comprise long-term data accumulated as a by-product of the MACHO Project, and high-speed, white-light photometry of a single eclipse. We (i) derive an improved ephemeris of T0 = HJD 245 0111.5144(3) + 0.442 677 14(6)E for the time of minimum light, (ii) find the eclipse structure to be stable over a period o...
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Key words
accretion, accretion discs,binaries: close,binaries: spectroscopic,stars: individual: CAL 87,Magellanic Clouds,X-rays: stars
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