Within the current uncertainties in the treatment of the coupling between pulsation and convection, limiting amplitude, nonlinear, convective models appear the only viable approach for providing theoretical predictions about the intrinsic properties of radial pulsators. In this paper we present the results of a comprehensive set of Cepheid models computed within such theoretical framework for selected assumptions on their original chemical composition
We present the results of non-linear pulsation modeling of bump Cepheids in the LMC and SMC. By obta...
We present a theoretical investigation on periods and amplitudes of RR Lyrae pulsators by adopting...
Classical Cepheid variable stars (from hereon: Cepheids) are high-sensitivity probes of stellar evol...
We present a new extended and detailed set of models for classical Cepheid pulsators at solar chemic...
In spite of the relevance of classical Cepheids as primary distance indicators, a general consensus ...
The numerical hydrodynamic modelling of beat Cepheid behavior has been a longstanding quest in which...
Context. With their period-luminosity relation, “classical Cepheids” (CC) are the most common primar...
We present a new extended and detailed set of models for Classical Cepheid pulsators at solar chemic...
Numerical experiments are conducted with a view toward constructing Cepheid models which satisfy obs...
Context. With their period-luminosity relation, "classical Cepheids" ( CC) are the most common prima...
Classical Cepheids and RR Lyrae are very important primary distance indicators and stellar populatio...
We present the results of an extensive theoretical investigation on the pulsation behavior of Bump C...
We present and discuss theoretical pulsational predictions concerning the properties of Classical Ce...
Some important problems in the theory of Cepheids and of other types of variables are pointed out. T...
We present the results of a theoretical investigation aimed at testing whether full amplitude, nonli...
We present the results of non-linear pulsation modeling of bump Cepheids in the LMC and SMC. By obta...
We present a theoretical investigation on periods and amplitudes of RR Lyrae pulsators by adopting...
Classical Cepheid variable stars (from hereon: Cepheids) are high-sensitivity probes of stellar evol...
We present a new extended and detailed set of models for classical Cepheid pulsators at solar chemic...
In spite of the relevance of classical Cepheids as primary distance indicators, a general consensus ...
The numerical hydrodynamic modelling of beat Cepheid behavior has been a longstanding quest in which...
Context. With their period-luminosity relation, “classical Cepheids” (CC) are the most common primar...
We present a new extended and detailed set of models for Classical Cepheid pulsators at solar chemic...
Numerical experiments are conducted with a view toward constructing Cepheid models which satisfy obs...
Context. With their period-luminosity relation, "classical Cepheids" ( CC) are the most common prima...
Classical Cepheids and RR Lyrae are very important primary distance indicators and stellar populatio...
We present the results of an extensive theoretical investigation on the pulsation behavior of Bump C...
We present and discuss theoretical pulsational predictions concerning the properties of Classical Ce...
Some important problems in the theory of Cepheids and of other types of variables are pointed out. T...
We present the results of a theoretical investigation aimed at testing whether full amplitude, nonli...
We present the results of non-linear pulsation modeling of bump Cepheids in the LMC and SMC. By obta...
We present a theoretical investigation on periods and amplitudes of RR Lyrae pulsators by adopting...
Classical Cepheid variable stars (from hereon: Cepheids) are high-sensitivity probes of stellar evol...