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- W2070745847 abstract "Data given and analyzed recently by Coulson et al. (1986) and Gieren (1982) provide a consistent set of Wesselink radii and Wesselink masses, for which the internal error bars appear to be small enough that a quantitative discussion appears to be warranted. When it is assumed that all Cepheids pulsate in the fundamental mode, a steep discontinuity in mass is found for periods around 6.5 days. When short-period Cepheids are interpreted as first-overtone pulsators as required theoretically (Christy, 1966; Stobie, 1969), the discontinuity disappears and the mass-period relation passes through the bump and beat masses for Cepheids." @default.
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- W2070745847 date "1988-01-01" @default.
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- W2070745847 title "Are most short-period Cepheids overtone pulsators?" @default.
- W2070745847 doi "https://doi.org/10.1086/185083" @default.
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