Photometry of the eclipsing binary SAO 189111.

Details Photometry of the eclipsing binary SAO 189111. Photometry of the eclipsing binary SAO 189111.

Dec 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994soust..36...87b&link_type=abstract

South. Stars, Vol. 36, No. 1 - 2, p. 87 - 90

Computer Science

Eclipsing Binaries: Photometry, Eclipsing Binaries: Light Curves

Scientific paper

The variability of SAO 189111 is reviewed and additional observations
described. The light curve, folded on a period of 1.1775 days, indicates
the star to be an eclipsing binary system. This is consistent with its
reported composite spectral type.

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