WW Aurigae / WW Aur
A number of observations were made with the Bradford Robotic Telescope Cluster Camera (BRT) between 2014 November 8 and 2016 January 11, using a tri-colour green filter.
Primary minimum of the EA type eclipsing binary, observed using the 2" Titan at Somerby Observatory, on 2019 January 17. The images were unfiltered.
Secondary minimum observed on 2019 February 25 using the 2" Titan at Somerby Observatory. The images were unfiltered.
A more complete primary minimum was observed on 2019 December 1, again from Somerby Observatory with the 2" Titan, stopped down to 1 " (25mm). The images were unfiltered.
Combining all the above observations generated the following light curve and phase diagram. The BRT observations are in red, the Somerby observations are in black.
The catalogue period for this star is 2.52501936d (GCVS), 2.52501922 (AAVSO VSX) and 2.52501943d (Kreiner). There is little o-c activity evident with this star (Kreiner). (Accessed 2019 January 18.)
[This page updated 2019 December 5.]