Transition probabilities for forbidden Fe II infrared lines

Details Transition probabilities for forbidden Fe II infrared lines Transition probabilities for forbidden Fe II infrared lines

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...193..327n&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 193, no. 1-2, March 1988, p. 327-333.

Astronomy and Astrophysics

Astrophysics

161

Abundance, Infrared Spectra, Metallicity, Scattering Cross Sections, Supernova Remnants, Transition Probabilities, Eigenvalues, Hamiltonian Functions, Iron, Nickel, Schroedinger Equation

Scientific paper

Transition probabilities are calculated for the lowest four terms of
Fe(+) in a 12-configuration basis. The construction of the
eigenfunctions is shown. The use of infrared line ratios for determining
electron temperature and density is briefly discussed.

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