2002MNRAS.331..389W


Query : 2002MNRAS.331..389W

2002MNRAS.331..389W - Mon. Not. R. Astron. Soc., 331, 389-393 (2002/April-1)

Effective collision strengths for fine-structure forbidden transitions among the 3s2 3p4 levels of ClII.

WILSON N.J. and BELL K.L.

Abstract (from CDS):

The ab initio R -matrix method is used to calculate effective collision strengths for electron-impact excitation of the sulphur-like ion Clii in the close-coupling approximation. All 10 astrophysically important fine-structure forbidden transitions within the 3s2 3p4 (formula), (formula), (formula) ground configuration levels are considered. The 12 lowest LS target states are included in the calculation. Effective collision strengths are obtained by averaging the electron collision strengths over a Maxwellian distribution of electron velocities.
Result. are presented for electron temperatures in the range logT (K)=3.3 to logT (K)=5.5, appropriate for astrophysical applications. These are the only effective collision strength data that are currently available.

Abstract Copyright: 2002 Blackwell Science Ltd

Journal keyword(s): atomic processes - line: formation - methods: analytical

Errata: Erratum vol. 338, p. 544 (2003)

Simbad objects: 3

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Number of rows : 3
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NGC 2440 PN 07 41 55.34603 -18 12 30.4117   11.469 10.104     ~ 665 2
2 IC 4634 PN 17 01 33.5816774904 -21 49 33.015515916   12.3 11.3     O3If 286 0
3 NGC 6543 PN 17 58 33.4039587288 +66 37 58.750734000   11.09 11.28     [WC] 1197 2

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