Revised Periods for QS Geminorum and V367 Geminorum

Details Revised Periods for QS Geminorum and V367 Geminorum Revised Periods for QS Geminorum and V367 Geminorum

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007pasp..119..274h&link_type=abstract

The Publications of the Astronomical Society of the Pacific, Volume 119, Issue 853, pp. 274-283.

Astronomy and Astrophysics

Astronomy

Stars: Binaries: Eclipsing, Stars: Individual (Qs Gem), Stars: Individual (V367 Gem)

Scientific paper

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.

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