| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1772358 | High Energy Density Physics | 2014 | 4 Pages |
Abstract
We report on recent efforts to generate high quality, self-consistent atomic physics models for L-shell ion stages for iron and the use of these data in collisional-radiative modeling of X-ray spectra of supernova remnants. As a specific example, we present comparisons between observed and theoretical X-ray spectra produced by Tycho's supernova remnant.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Astronomy and Astrophysics
Authors
C.J. Fontes, K.A. Eriksen, J. Colgan, H.L. Zhang, J.P. Hughes,