An Examination of the delta Scuti Variable GW Draconis

Details An Examination of the delta Scuti Variable GW Draconis An Examination of the delta Scuti Variable GW Draconis

Dec 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aas...203.0804m&link_type=abstract

American Astronomical Society Meeting 203, #08.04; Bulletin of the American Astronomical Society, Vol. 35, p.1217

Astronomy and Astrophysics

Astronomy

Scientific paper

The period of GW Dra has been established to be 0.1261875d. There are at least 4 significant frequencies in this multiperiodic δ Scuti. At least one of these frequencies yields a period that is longer than those accepted for δ Scuti stars. It is a possible g-mode pulsation in a δ Scuti. The amplitude of variation in R and I has also been determined as well as the radial velocity amplitude. The colors R-I and V-R have been calculated and the magnitudes have been standardized using SA 110, SA 112, and SA 114.

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