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The Period-Luminosity and the Period-Spectrum Relations of Cluster-Type Cepheids.

Paris Pismis

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Abstract

The results of the present discussion are based on the material of M. Schwarzschild for 43 cluster-type variables of types a and b in the globular cluster M 3. It is pointed out that the color-magnitude diagram of these variables shows a descending branch resembling that of the main sequence. It is shown that this characteristic, combined with the theoretical period-density relation (satisfied by these variables), gives, as a consequence, the period-spectrum and the period-luminosity relations

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The results of the present discussion are based on the material of M. Schwarzschild for 43 cluster-type variables of types a and b in the globular cluster M 3. It is pointed out that the color-magnitude diagram of these variables shows a descending branch resembling that of the main sequence. It is shown that this characteristic, combined with the theoretical period-density relation (satisfied by these variables), gives, as a consequence, the period-spectrum and the period-luminosity relations

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Available abstract

The results of the present discussion are based on the material of M. Schwarzschild for 43 cluster-type variables of types a and b in the globular cluster M 3. It is pointed out that the color-magnitude diagram of these variables shows a descending branch resembling that of the main sequence. It is shown that this characteristic, combined with the theoretical period-density relation (satisfied by these variables), gives, as a consequence, the period-spectrum and the period-luminosity relations

Key concepts: Cepheid variable, Physics, Period (music), Astrophysics, Luminosity, Cluster (spacecraft), Globular cluster, Astronomy

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