Revised Periods for QS Geminorum and V367 Geminorum

Abstract

We have examined the field around the variable stars QS Geminorum and V367 Geminorum. For the δ Scuti-type variable QS Gem, we determined a revised period of 0.1346116 days, which is close to the originally published period from Hipparcos. For the eclipsing system V367 Gem, we found a period of 0.6992285 days, which is substantially different from the published value. In addition, we report five suspected variable stars in the field: one is a long-period eclipsing system, one a likely γ Doradus star, and the other three are of unknown type.