Simulations of early F-type to late A-type main-sequence and sub-giant stars
1 : Univ. Appl. Sciences Technikum Wien; and University of Vienna
2 : Univ. Appl. Sciences Technikum Wien; and WPI, c/o University of Vienna
3 : University of Vienna
4 : University of Texas at Austin
We present preliminary results of supercomputer simulations of stellar atmospheres warmer than the Sun (with effective temperatures of up to 9000 K) obtained with the ANTARES numerical code.
The data will be used as benchmark to improve multi-dimensional radiation-hydrodynamic modeling for this type of stellar objects and as the basis for computations of synthetic spectra and other observable signatures of the characteristic physical properties of relevant stars.
| Subject : | : | Poster |
| Topics | : | D1 - Advances in stellar physics: Chemical composition and opacities |
| PDF version | : |  PDF version |
