The RRd masses revisited

Details The RRd masses revisited The RRd masses revisited

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...376..717s&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 376, Aug. 1, 1991, p. 717-720.

Astronomy and Astrophysics

Astrophysics

11

Stellar Interiors, Stellar Mass, Stellar Oscillations, Cepheid Variables, Metallicity, Star Clusters

Scientific paper

The RRd mass determination is reexamined using both new and previously
existing linear pulsation models. The weight of evidence remains
strongly with the 'canonical' values (0.55 solar mass for Oosterhoff I
clusters and 0.65 solar mass for Oosterhoff II clusters), unless the
Population II metal opacities turn out to be very high.

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