Astronomy and Astrophysics – Astrophysics
Scientific paper
Jun 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004a%26a...420..763b&link_type=abstract
Astronomy and Astrophysics, v.420, p.763-768 (2004)
Astronomy and Astrophysics
Astrophysics
14
Atomic Data, Line: Formation, Ism: Abundances, Atomic Processes, Ism: Hii Regions
Scientific paper
We study the effects of using a \bar{4d} pseudo-orbital on the collision strengths for electron impact excitations of forbidden transitions in NiII computed in the close coupling approximation. It is found that the resonance structures of the collision strengths are quite sensitive to the way the pseudo-orbital is created. Further, the close coupling expansion with a single \bar4d orbital does not converge, resulting in a poor representation of (N+1)-electrons auto-ionizing states. Much greater expansions are needed to properly represent resonance structures in electron impact excitation calculations, resulting in variations of up to factors of two, with respect to previous computations, in the Maxwellian averaged excitation rate coefficients.
Tables \ref{t1} and \ref{t2} are also available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/420/763
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