  First photometric study for the newly discovered systems USNO-B1.0
1091-0130715 and GSC-03449-0680 were applied by means of recent windows
interface version of the Wilson and Devinney code based on model atmospheres by
Kurucz (1993). The accepted models reveal some absolute parameters for both
systems, which used in adopting the spectral type of the systems components and
follow their evolutionary status. Distances to each systems are and physical
properties are estimated. Comparisons of the computed physical parameters with
stellar models are discussed.
