Beta Cephei stars in open clusters as metallicity indicators

Details Beta Cephei stars in open clusters as metallicity indicators Beta Cephei stars in open clusters as metallicity indicators

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.169..117d&link_type=abstract

(IAU, European Regional Astronomy Meeting on New Windows to the Universe, 11th, La Laguna, Spain, July 3-8, 1989) Astrophysics a

Astronomy and Astrophysics

Astrophysics

1

Metallicity, Open Clusters, Stellar Oscillations, B Stars, Hertzsprung-Russell Diagram, Solar Neighborhood

Scientific paper

The content of Beta Cephei pulsating stars in young open clusters is examined. The actual metallicity differences between clusters are suggested to be detectable as variations of the location of these stars in the photometric diagrams. A quantitative estimate of these differences is made and attention is given to the existence and possible determination of a metallicity gradient in the galactic plane.

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