Megallanic Cloud cepheids - Abundances, reddenings, P-L and P-L-C relations - A review

Details Megallanic Cloud cepheids - Abundances, reddenings, P-L and P-L-C relations - A review Megallanic Cloud cepheids - Abundances, reddenings, P-L and P-L-C relations - A review

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984iaus..108..157f&link_type=abstract

IN: Structure and evolution of the Magellanic Clouds; Proceedings of the Symposium, Tuebingen, West Germany, September 5-8, 1983

Computer Science

37

Cepheid Variables, Interstellar Extinction, Magellanic Clouds, Stellar Composition, Abundance, Infrared Spectra, Stellar Color

Scientific paper

The cepheid variables of the Magellanic Clouds are characterized in a review of recent observational and statistical investigations. Topics examined include the rapid growth in the number of cepheids detected and in the number of observations available for analysis, problems in the determination of Fe/H abundance ratios, methods used to estimate reddening and absorption, and the period-luminosity and period-luminosity-color relationships in the BV and IR spectral ranges.

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