| Issue |
Astron. Astrophys. Suppl. Ser.
Volume 126, Number 2, December I 1997
|
|
|---|---|---|
| Page(s) | 373 - 378 | |
| DOI | https://doi.org/10.1051/aas:1997388 | |
| Published online | 15 December 1997 | |
Atomic data from the Iron Project*
XXVII. Electron impact excitation collision strengths and rate coefficients for Fe IV
Department of Astronomy, The Ohio State University, Columbus, OH 43210, U.S.A.
Send offprint request to: H.L. Zhang
Received:
28
February
1997
Accepted:
3
March
1997
Abstract
Collision strengths and maxwellian-averaged rate coefficients
have been calculated for 8771 non-vanishing
transitions among 140 fine structure levels, dominated by the
configurations
,
, and
in Fe IV.
Collision strengths are calculated
using the R-matrix method with a 49 term
close-coupling target expansion for electron energies up to 15
rydbergs.
Rate coefficients are tabulated for a wide range of temperatures
in which Fe IV is abundant in plasma sources.
A brief discussion of the calculations and sample results are given.
The present rates for Fe IV are
expected to find applications in
spectral diagnostics of a variety of astrophysical sources.
Key words: atomic processes / planetary nebulae: general / H II regions
Table 3 for complete data for Fe IV is only available in electronic form at the CDS via anonymous to ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/Abstract.html
© European Southern Observatory (ESO), 1997
