Abstract
We present preliminary results derived from the data obtained during five observing campaigns in 2001, 2003, 2004, 2006 and 2007, of the δ Set-type variable star 67 UMa, at Sierra Nevada Observatory, Spain. The analysis of the data was performed by means of the Fourier Transform method, and results are shown. The intrinsic b-y, m1, c1 values are derived and the physical parameters are determined. © 2008 IOP Publishing Ltd.
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CITATION STYLE
Rolland, A., López De Coca, P., Costa, V., Rodríguez, E., & Olivares, I. (2008). Strömgren photometry of the δ Scuti star 67 UMa. In Journal of Physics: Conference Series (Vol. 118). Institute of Physics Publishing. https://doi.org/10.1088/1742-6596/118/1/012070
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