A CCD light curve of PG 0818 + 513

Details A CCD light curve of PG 0818 + 513 A CCD light curve of PG 0818 + 513

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990acasn..31..305c&link_type=abstract

(Acta Astronomica Sinica, vol. 31, no. 3, 1990, p. 305-308) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 14, Dec. 1

Astronomy and Astrophysics

Astrophysics

2

Cataclysmic Variables, Charge Coupled Devices, Eclipsing Binary Stars, Light Curve, Stellar Spectrophotometry, Astronomical Catalogs, Stellar Orbits, Stellar Spectra

Scientific paper

High-speed CCD photometry (time resolution 63 s) was obtained of PG 0818
+ 513 on March 27, 1989 and April 2, 1989, and two complete light curves
were derived. This object is proved to be a cataclysmic eclipsing binary
with an orbital period of 0.1559 d.

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