A check on EU Tauri

Details A check on EU Tauri A check on EU Tauri

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pasp...99.1093f&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 99, Oct. 1987, p. 1093-1096.

Astronomy and Astrophysics

Astronomy

4

Astronomical Photometry, Cepheid Variables, Light Curve, Taurus Constellation, Stellar Color, Stellar Magnitude, Stellar Oscillations

Scientific paper

New uvby beta RI photometry has been obtained to check the suggestion of Gieren and Matthews (1987) 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.

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