A survey of Cepheid sizes
J. D. Fernie
Abstract
J. D. Fernie
Abstract
The radius is one of the fundamental physical parameters governing a Cepheid's pulsation. If the radius of a Cepheid can be established independently of its luminosity and temperature, that radius, combined with a temperature scale, can yield the Cepheid's luminosity. The Baade-Wesselink (BW) method provides an approach for determining a Cepheid's radius independently of any temperature or luminosity scale. In connection with the present investigation, data regarding individual BW radius determinations are provided in a table. The best BW radii are selected and a period-radius (P-R) relation is determined. The obtained relation is compared to theoretical P-R relations. The BW and theoretical relations are compared to one obtained from the luminosities and temperatures of Cepheids in open clusters and associations.
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The radius is one of the fundamental physical parameters governing a Cepheid's pulsation. If the radius of a Cepheid can be established independently of its luminosity and temperature, that radius, combined with a temperature scale, can yield the Cepheid's luminosity. The Baade-Wesselink (BW) method provides an approach for determining a Cepheid's radius independently of any temperature or luminosity scale. In connection with the present investigation, data regarding individual BW radius determinations are provided in a table. The best BW radii are selected and a period-radius (P-R) relation is determined. The obtained relation is compared to theoretical P-R relations. The BW and theoretical relations are compared to one obtained from the luminosities and temperatures of Cepheids in open clusters and associations.
Key concepts: Cepheid variable, Physics, Astrophysics, RADIUS, Luminosity, Hertzsprung–Russell diagram, Open cluster, Astronomy