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Radius Determination for Nine Short Period Cepheids
Published online by Cambridge University Press: 12 April 2016
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From November, 1981 to March, 1982, nine Pop I and Pop II cepheids of periods between 1.5 and 4.2 days have been monitored, in Geneva photometry from La Silla Observatory (Chile) and in radial velocities from the Haute-Provence Observatory (France). These cepheids are listed in Table 1. Figure 1 shows an example of the light, colour and velocity curves for EU Tau, a small amplitude cepheid with a period of 2.10 days.
- Type
- Part I. Fundamental Parameters
- Information
- International Astronomical Union Colloquium , Volume 82: Cepheids: Theory and Observations , 1985 , pp. 34 - 37
- Copyright
- Copyright © Cambridge University Press 1985
References
Wolley, R., Carter, B.: 1973, Monthly Not. R. Astron. Soc.
162, 379
10.1093/mnras/162.4.379CrossRefGoogle Scholar