Physics
Scientific paper
Nov 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008pzp.....8...34g&link_type=abstract
Peremennye Zvezdy Prilozhenie, vol.8, no. 34.
Physics
Scientific paper
Nicholson and Scottish (2006) wrote that this star is an EB eclipser of
1.8347 day period using NSVS data. In fact those self same data
actually show the period to be 11.8 days and the star to be a rotational
variable.
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