Binary systems with black hole component

The LIGO detection of gravitational waves in the year of 2015 from a system with two stellar black hole components make the systems with black hole components important sources to study fundamentals of physics. In this thesis, binary systems with a main-sequence/evoloved star and a black hole have been studied. It has been catalogued the orbital and physical parameters of 27 binary systems of whose parameters are relatively known to be accurate. It is discussed angular momentum mechanisms, the gravitational radiation and magnetised stellar winds, and using these catalogued parameters it is studied what angular momentum mechanisms to be important in these systems. Finally, the new photometric varionations of some of the observable systems have been obtained with the T60 and T100 telescopes. Short and long period photometric behaviours of these selected systems are studied.