Level populations for Be-sequence ions in astrophysical plasmas
Abstract
Level populations for the 10 n = 2 states of ions in the Be-sequence from C III to Si XI are presented. The results are for two ranges of electron density (Ne = 108 - 1013cm-3 and Ne = 102 - 107cm-3), the former applicable to the solar corona and transition region and the latter to other astrophysical objects such as quasars and Seyfert galaxies.
- Publication:
-
Monthly Notices of the Royal Astronomical Society
- Pub Date:
- March 1984
- DOI:
- 10.1093/mnras/207.3.459
- Bibcode:
- 1984MNRAS.207..459K
- Keywords:
-
- Atomic Energy Levels;
- Beryllium;
- Cosmic Plasma;
- Electron States;
- Isoelectronic Sequence;
- Cosmochemistry;
- Electron Density (Concentration);
- Quasars;
- Seyfert Galaxies;
- Solar Corona;
- Astrophysics