Abstract
Aims. In this paper we report calculations for energy levels, radiative rates, collision strengths, and effective collision strengths for transitions in Fe XVI. Methods. For energy levels and radiative rates we have used the General purpose Relativistic Atomic Structure Package ( grasp), and for the compuations of collision strengths the Dirac Atomic R-matrix Code (darc) has been adopted. Results. Energies for the lowest 39 levels among the n
| Original language | English |
|---|---|
| Pages (from-to) | 1249-1257 |
| Number of pages | 9 |
| Journal | Astronomy and Astrophysics |
| Volume | 450 |
| Issue number | 3 |
| Publication status | Published - May 2006 |
ASJC Scopus subject areas
- Space and Planetary Science