56 citations · 287 across the 17 of their papers we have counts for
17 papers
Scaling of oscillation frequencies in rotating stars
Diego Castañeda, Robert G. Deupree
Properties of stars undergoing pulsation such as the well known root-mean-density scaling relation can be useful when trying to match the observed properties of a particular star.…
Radial Stellar Pulsation and Three-Dimensional Convection. IV. Full Amplitude Three-Dimensional Solutions
Christopher M. Geroux, Robert G. Deupree
Three dimensional hydrodynamic simulations of full amplitude RR Lyrae stars have been computed for several models across the instability strip. The three dimensional nature of the…
Modelling observable properties of rapidly rotating stars
Diego Castañeda, Robert G. Deupree, Jason P. Aufdenberg
To fully understand the Be star phenomenon, one must have a reasonable degree of knowledge about the star beneath the disk, which is often found to be rapidly rotating. Rapid rotat…
Scaling of Observable Properties in Rapidly Rotating Stars
D. Castañeda, R. G. Deupree
The spectral energy distribution as a function of inclination is computed using 2D rotating stellar models and NLTE plane parallel stellar atmospheres. These models cover the range…
Radial Stellar Pulsation and Three-Dimensional Convection. III. Comparison of Two-Dimensional and Three-Dimensional Convection Effects on Radial Pulsation
Christopher M. Geroux, Robert G. Deupree
We have developed a multidimensional radiation hydrodynamics code to simulate the interaction of radial stellar pulsation and convection for full amplitude pulsating models. Convec…
Radial Stellar Pulsation and Three-Dimensional Convection. II. Two-Dimensional Convection In Full Amplitude Radial Pulsation
Chris M. Geroux, Robert G. Deupree
We have developed a three-dimensional radiation hydrodynamics code to simulate the interaction of convection and radial pulsation in classical variable stars. One key goal is the a…