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| Paper: |
Atomic Data in Non-LTE Model Stellar Atmospheres |
| Volume: |
288, Stellar Atmosphere Modeling |
| Page: |
117 |
| Authors: |
Lanz, T.; Hubeny, I. |
| Abstract: |
Extensive sources of atomic data are required to calculate NLTE line-blanketed model atmospheres. I will discuss their implementation in our NLTE model atmosphere code, TLUSTY, and in our spectrum synthesis code, SYNSPEC, with a particular attention to the statistical methods required to incorporate the opacity of iron-peak elements. A few typical results and comparisons to other codes will be shown. |
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