Abstract
The modeling of the radiation transport in supernova atmospheres is discussed in terms of lightcurve physics and spectral synthesis. The importance of accurate and complete atomic physics is discussed. The elements and ionization stages which are important for supernova calculations are listed as well as the processes for which data are required.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 125-127 |
| Number of pages | 3 |
| Journal | Physica Scripta T |
| Volume | 83 |
| State | Published - 1999 |
ASJC Scopus subject areas
- Atomic and Molecular Physics, and Optics
- Mathematical Physics
- Condensed Matter Physics
- General Physics and Astronomy