Abstract:
U, B, V photometry of the Eclipsing binary system DX Aqr has been presented for the first time. The period of the system comes out to be nearly half the period given by Strohmeier (1966) and a value of 0ͩ.472502 has been determined. The colour of the system has been discussed. The primaru eclipse is a total occulation. The orbit seems to be eccentric. The system belongs to Algol type. DX Aqr may be a very complicated system. The present results are considerably different from those of earlier investigations.
