OBJECTIVE
In 95% of patients with primary biliary cirrhosis (PBC) antimitochondrial antibodies (AMAs) can be detected reacting with at least one of the five components of the M2 antigen identified asâ€¦ (More)

The physical and numerical ingredients of the Vienna nonlinear model for radially pulsating stars are presented. Stellar pulsations are investigated by solving the full system of radiationâ€¦ (More)

The Vienna nonlinear code for modelling pulsating stars is applied to the problem of RR Lyrae double mode pulsation. For stellar parameters of M = 0.65 M , log(L/L ) = 1.72 and XYZ=(0.760, 0.239,â€¦ (More)

The luminosities, effective temperatures and metallicities that are derived empirically by KovÃ¡cs and Jurcsik from the light curves of a large number of globular cluster and field RRab and RRc starsâ€¦ (More)

A hydrodynamical survey of the pulsational properties of first overtone Galactic Cepheids is presented. The goal of this study is to reproduce their observed lightand radial velocity curves. Theâ€¦ (More)

By performing detailed frequency-dependent radia-tive transfer computations we have obtained UBVI light curves of nonlinear RR Lyrae models, which recently have been calculated by the Viennaâ€¦ (More)

Using an adaptive radiation hydrodynamics code we have computed a grid of fundamental mode RR Lyrae models in order to give a detailed comparison to observed RR Lyrae light curves and to investigateâ€¦ (More)

The fundamental mode RR-Lyrae light and radial velocity curves presented in Feuchtinger & Dorfi (1994) are Fourier analysed and compared to observational data and other theoretical investigations.â€¦ (More)

The Vienna nonlinear convective pulsation code is applied to the case of RR Lyrae stars. Assuming two sets of stellar parameters (M = 0.65M , L = 52.5 L , Z = 0.001 and M = 0.75 M , L = 52.5 L , Z =â€¦ (More)