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A CHECK ON EU TAURI
J. D. FERNIE
Publications of the Astronomical Society of the Pacific
Vol. 99, No. 620 (October 1987), pp. 1093-1096
Published by: Astronomical Society of the Pacific
Stable URL: http://www.jstor.org/stable/40679034
Page Count: 4
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New uvby βRI photometry has been obtained to check the suggestion of Gieren and Matthews (1987a, b) that the two-day classical Cepheid EU Tau had changed its period slightly and also showed a secondary period half the primary period. The present photometry does not support this suggestion. The earlier period is confirmed and improved, and there is no evidence of a secondary period. An improved color excess is derived, and this, when compared to values from a period-color relation, supports the view that EU Tau is an overtone pulsator.
Publications of the Astronomical Society of the Pacific © 1987 The University of Chicago Press