We give a brief overview of Cepheids and of their modeling, with particular emphasis on F/O1 Beat Cepheids. Then we revisit the use of Period Ratio vs. Period diagram (Petersen diagram) for fundamental/first overtone Beat Cepheids, because they allow one to put very tight constraints on their metallicity Z. The Petersen diagram is shown to be largely independent of the helium content Y, of the mass-luminosity relation that is used in their construction, and of stellar rotation rates. However, it shows sensitivity to the chemical makeup of the elements that are lumped into the metallicity parameter Z. The Petersen diagram for the new Asplund, M., Grevesse, N., & Sauval, A.J. (2005, ASP Conf. Ser., 336, 25) solar mix is compared to that for f...
Accurate mass determinations for Cepheids may be used to determine the degree of excess mixing in th...
Context. Physical and phenomenological properties (radius, luminosity, shape of the light curve, etc...
We have assessed the influence of the stellar iron content on the Cepheid Period–Luminosity (PL) rel...
The mere location of a Beat Cepheid model in a Period Ratio vs. Period diagram (Petersen diagram) pu...
We determine the metallicity and detailed chemical abundances (α, iron-peak and neutron-capture elem...
Context. Classical Cepheids are the most popular distance indicators and tracers of young stellar po...
Classical Cepheids are the most popular distance indicators and tracers of young stellar populations...
The Cepheid Period-Luminosity relation is unquestionably one of the most powerful tools at our dispo...
Context. Classical Cepheids (DCEPs) represent a fundamental tool to calibrate the extragalactic dist...
International audienceContext. Classical Cepheids are the most popular distance indicators and trace...
International audienceWe have assessed the influence of the stellar iron content on the Cepheid Peri...
Context. Classical Cepheids (DCEPs) are the most important primary indicators for the extragalactic ...
Context. The ratio of the first overtone (1O)/fundamental (F) periods of mixed-mode Cepheids that pu...
We present results based on a Baade-Wesselink analysis of Cepheids in the Small Magellanic Cloud. Th...
We have applied the near-IR Barnes-Evans realization of the Baade-Wesselink method as calibrated by ...
Accurate mass determinations for Cepheids may be used to determine the degree of excess mixing in th...
Context. Physical and phenomenological properties (radius, luminosity, shape of the light curve, etc...
We have assessed the influence of the stellar iron content on the Cepheid Period–Luminosity (PL) rel...
The mere location of a Beat Cepheid model in a Period Ratio vs. Period diagram (Petersen diagram) pu...
We determine the metallicity and detailed chemical abundances (α, iron-peak and neutron-capture elem...
Context. Classical Cepheids are the most popular distance indicators and tracers of young stellar po...
Classical Cepheids are the most popular distance indicators and tracers of young stellar populations...
The Cepheid Period-Luminosity relation is unquestionably one of the most powerful tools at our dispo...
Context. Classical Cepheids (DCEPs) represent a fundamental tool to calibrate the extragalactic dist...
International audienceContext. Classical Cepheids are the most popular distance indicators and trace...
International audienceWe have assessed the influence of the stellar iron content on the Cepheid Peri...
Context. Classical Cepheids (DCEPs) are the most important primary indicators for the extragalactic ...
Context. The ratio of the first overtone (1O)/fundamental (F) periods of mixed-mode Cepheids that pu...
We present results based on a Baade-Wesselink analysis of Cepheids in the Small Magellanic Cloud. Th...
We have applied the near-IR Barnes-Evans realization of the Baade-Wesselink method as calibrated by ...
Accurate mass determinations for Cepheids may be used to determine the degree of excess mixing in th...
Context. Physical and phenomenological properties (radius, luminosity, shape of the light curve, etc...
We have assessed the influence of the stellar iron content on the Cepheid Period–Luminosity (PL) rel...