Published July 1, 1985
| Version v1
Journal article
C II emission lines formed in optically thin plasmas
- 1. Department of Pure and Applied Physics, The Queen's University of Belfast
Description
New Einstein A-coefficients and electron impact collision rates are presented for transitions between the three lowest ls of C II. The former are based on complex configuration interaction wave functions, while the latter use such wave functions in an eight-state R-matrix calculation of the collision process. These new atomic data are then used to calculate populations for the corresponding seven fine-structure levels on the assumption of an isotropic optically thin plasma. Theoretical emission-line intensity ratios deduced from these populations are in excellent agreement with observed low- and high-density limits
Additional details
Publishing Information
- Journal Title
- Astrophys. J.
- Journal Volume
- 294
- Journal Issue
- 1
- Series
- Astrophys. J.
- Journal Page Range
- 200-206
- ISSN
- 0004-637X
- CODEN
- ASJOA
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 17014080
- Subject category
- S74: ATOMIC AND MOLECULAR PHYSICS;
- Resource subtype / Literary indicator
- Numerical Data
- Descriptors DEI
- CARBON IONS; CONFIGURATION INTERACTION; EINSTEIN COEFFICIENTS; ELECTRON-ION COLLISIONS; EMISSION SPECTRA; ENERGY-LEVEL DENSITY; FINE STRUCTURE; OSCILLATOR STRENGTHS; PLANETARY NEBULAE; PLASMA; R MATRIX; THEORETICAL DATA; ULTRAVIOLET SPECTRA; WAVE FUNCTIONS
- Descriptors DEC
- ATOMIC IONS; CHARGED PARTICLES; COLLISIONS; DATA; ELECTRON COLLISIONS; FUNCTIONS; INFORMATION; ION COLLISIONS; IONS; MATRICES; NEBULAE; NUMERICAL DATA; SPECTRA