Kurucz ODFNEW /NOVER models. Newly computed ODFs with better opacities and better abundances have been used. (The convective treatment is described in Castelli et al. 1997, AA 318, 841.)
The LCA is dedicated to advancing the state-of-the-art of astrophysical simulation through the development and dissemination of community codes, and through large-scale simulations of astrophysical and cosmological systems. Our community codes include the ZEUS family of astrophysical MHD codes, and ENZO, an adaptive mesh hydrodynamic cosmological code. We also offer a new, elliptic equation, multigrid solver MGMPI. Members and collaborators of the LCA apply ZEUS and ENZO to a wide variety of fluid dynamical probelms in astrophysics and cosmology.
A grid of LTE and non-LTE synthetic spectra of hot DA white dwarfs. It covers Teff from 17,000 K to 100,000 K and log(g) from 7.0 to 9.5. The stellar models are built for pure hydrogen and the spectra cover a wavelength range from 90 nm to 2.5 micron.