Period-magnitude relationships for fundamental and first overtone Cepheids

Details Period-magnitude relationships for fundamental and first overtone Cepheids Period-magnitude relationships for fundamental and first overtone Cepheids

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001sf2a.conf..193a&link_type=abstract

Abstracts from SF2A-2001: Semaine de l'Astrophysique Francaise, meeting held in Lyon, France, May 28-June 1st, 2001, Eds.: F. Co

Astronomy and Astrophysics

Astrophysics

Scientific paper

We present theoretical period-magnitude relationship for Cepheids in different filters for fundamental and first overtone pulsators. These results are calculated taking into account the evolution, a linear stability analysis, atmosphere calculations and synthetic spectra in a consistant way. The results are provided for different metallicities characteristic of the Magellanic Clouds and the Milky Way. Comparison are made with observations from EROS and OGLE in the MC.

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