Poster title:  New near-IR curves modelling of newly discovered BHB binary stars

Poster abstract: We present new results in the study of selected Blue Horizontal Branch binary 
systems recently detected in the VVV Survey images in the Galactic bulge.
For the analysis of the Ks band light curve we used the “Physics Of Eclipsing Binaries” (PHOEBE 
1.0) interactive code. The selected sample consists of five Detached, Contact and Semi-detached  
candidates of eclipsing binaries. The systems discovered present orbital inclinations close to 80º, 
and have low eccentricities with surface temperatures range between 7000 and 12000 K.