A CCD light curve of the cataclysmic eclipsing binary PG 0027+260

Details A CCD light curve of the cataclysmic eclipsing binary PG 0027+260 A CCD light curve of the cataclysmic eclipsing binary PG 0027+260

Sep 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990cha%26a..14..359l&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 14, Issue 3, p. 359-360.

Astronomy and Astrophysics

Astrophysics

Stars-Eclipsing Binaries-Cataclysmic Variables

Scientific paper

On 1989 November 30 we carried out a high speed CCD photometry of PG
0027+260 with a time resolution of 108 s and obtained a complete light
curve, thereby confirming it to be a cataclysmic eclipsing binary with a
period of 0.146 d.

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