Revised Periods for QS Geminorum and V367 Geminorum We have examined the field around the variable stars QS Geminorum andV367 Geminorum. For the δ Scuti-type variable QS Gem, wedetermined a revised period of 0.1346116 days, which is close to theoriginally published period from Hipparcos. For the eclipsing systemV367 Gem, we found a period of 0.6992285 days, which is substantiallydifferent from the published value. In addition, we report fivesuspected variable stars in the field: one is a long-period eclipsingsystem, one a likely γ Doradus star, and the other three are ofunknown type.
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