Volume 550, February 2013
|Number of page(s)||2|
|Section||Atomic, molecular, and nuclear data|
|Published online||31 January 2013|
New effective recombination coefficients for nebular N ii lines⋆ (Corrigendum)
Department of AstronomySchool of Physics, Peking University,
2 Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, UK
3 Kavli Institute for Astronomy and Astrophysics, Peking University, 100871 Beijing, PR China
This article has no abstract.
Key words: atomic data / line: formation / HII regions / ISM: atoms / planetary nebulae: general / errata, addenda
Corrected Tables 3–15 are all available at the CDS via anonymous ftp to cdsarc.u-strasbg.fr(188.8.131.52) or via http://cdsweb.u-strasbg.fr/viz-bin/qcat?J/A+A/530/A18. Effective recombination coefficients at an extended temperature and density range are available from the authors.
© ESO, 2013
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