Taking into account results obtained from models and analyses, we determined
the nature and structures of V1003 Her. We analysed the light curves obtained
in this study together with the available radial velocity curve. The analysis
revealed that the inclination (i) of the system was found to be 45.82 (2.71),
while the semi-major axis (a) was computed as 2.925 (0.143) Rsun. The mass of
the primary component was found to be 1.204 (0.004) Msun, while it was obtained
as 0.450 (0.006) Msun for the secondary component. The radius of the primary
component was computed as 1.424 (0.001) Rsun, while it was computed as 0.904
(0.001) Rsun for the secondary component. The analysis indicates that there are
two spotted areas close to each other on the surface of the secondary
component. In addition, B-band light and B-V colour curves reveal that there is
a radiation excess toward the phase of 0.40. This should be caused due to some
heating of the surface by the events like thermal flare, or the structures like
plage. Finally, the analysis and model demonstrated that V1003 Her should be a
near-contact binary with high levelComment: 19 pages, 5 figures. arXiv admin note: text overlap with
arXiv:1210.428
