Add to ORKGWe reexamine the RRd mass determination using both new and previously existing linear pulsation models. Our conclusion is that the weight of evidence remains strongly with the canonical values (0.55 M ʘ for Oosterhoff I clusters and 0.65 M ʘ for Oosterhoff II clusters), unless the Population II metal opacities turn out to be very high
A theoretical study of Population II variables has been carried out using the nonlinear approach and...
We are revising the consistency of photometric metallicity formulae widely used for fundamental-mode...
We present new B-band CCD photometry for five double-mode RR Lyrae (RRd) variables (V68, V79, V87, V...
Some results are given from the comparison with observations of a large number of hydrodynamic pulsa...
We re-examine the double-mode RR Lyrae (RRd) mass determination using both new and previously existi...
The RR Lyrae stars play a role in the investigation of many important astronomical problems. For exa...
Hydrodynamic pulsation models are matched with observations of globular cluster RRc stars to derive ...
Masses, temperatures, and absolute luminosities are proposed for a large sample of RRc stars in the ...
In a recent study, Simon (1990) determined masses and temperatures for a large sample of RRc stars i...
Comparative linear nonadiabatic pulsation calculations are presented using the OPAL and Opacity Proj...
The horizontal-branch evolutionary tracks of Lee and Demarque (LD) are combined with the period/mean...
The results of nonlinear, convective models of RR Lyrae pulsators with metal content Z=0.0001 to 0.0...
We present a theoretical investigation on the pulsational behavior of metal-rich RR Lyrae variables ...
We present an analysis of the period-V-amplitude plane for RR0 Lyrae stars (fundamental mode pulsato...
Non-linear calculations of intermediate amplitude to investigate stability have been carried out for...
A theoretical study of Population II variables has been carried out using the nonlinear approach and...
We are revising the consistency of photometric metallicity formulae widely used for fundamental-mode...
We present new B-band CCD photometry for five double-mode RR Lyrae (RRd) variables (V68, V79, V87, V...
Some results are given from the comparison with observations of a large number of hydrodynamic pulsa...
We re-examine the double-mode RR Lyrae (RRd) mass determination using both new and previously existi...
The RR Lyrae stars play a role in the investigation of many important astronomical problems. For exa...
Hydrodynamic pulsation models are matched with observations of globular cluster RRc stars to derive ...
Masses, temperatures, and absolute luminosities are proposed for a large sample of RRc stars in the ...
In a recent study, Simon (1990) determined masses and temperatures for a large sample of RRc stars i...
Comparative linear nonadiabatic pulsation calculations are presented using the OPAL and Opacity Proj...
The horizontal-branch evolutionary tracks of Lee and Demarque (LD) are combined with the period/mean...
The results of nonlinear, convective models of RR Lyrae pulsators with metal content Z=0.0001 to 0.0...
We present a theoretical investigation on the pulsational behavior of metal-rich RR Lyrae variables ...
We present an analysis of the period-V-amplitude plane for RR0 Lyrae stars (fundamental mode pulsato...
Non-linear calculations of intermediate amplitude to investigate stability have been carried out for...
A theoretical study of Population II variables has been carried out using the nonlinear approach and...
We are revising the consistency of photometric metallicity formulae widely used for fundamental-mode...
We present new B-band CCD photometry for five double-mode RR Lyrae (RRd) variables (V68, V79, V87, V...