Orbital period changes of four neglected short-period semidetached Algols, SX Dra, AV Del, CU Peg and DK Peg, are presented
based on the analysis of their O–C observations. It is found that the three systems, AV Del, CU Peg and DK Peg, show rapid
period increase at rates of dP/dt =+3.15 × 10-6, +2.00 × 10-6 and +4.88 × 10-7days/year respectively. For the other system, SX Dra, a possible periodic
... [Show full abstract] variation in the orbital period is discovered to
superimpose on a very rapid period increase (dP/dt = +1.09 × 10-5 days/year). The period increases of the four Algols can be explained by a mass transfer from the secondary to the more massive
primary, which is in agreement with the semi-detached configurations of these systems. However, since the period increases
are rather rapid, the mass transfer should be on a dynamical time scale. The cyclic period change in SX Dra suggests that
there may exist a third body in this system.