The Gamma Doradus variables, a new class of pulsating stars. The case of HD 224945
Other publications > Other ยท 1996
Authors: Poretti, E., Akan, C., Bossi, M., Koen, C., Krisciunas, K., Rodriguez, E.
Other, International, 1996,
Summary
A multisite campaign involving five observatories allowed us to solve the light curve of the Gamma Doradus star HD 224945. The multiperiodic content, the high frequency term at 3.00 c/d and the frequency spacing between the observed terms strongly support its pulsational nature. Considering the low frequency terms observed in Gamma Dor stars, it seems that g--mode pulsators can be found near the cold border of the instability strip.