Improved radiative transition probabilities for O II forbidden lines

Details Improved radiative transition probabilities for O II forbidden lines Improved radiative transition probabilities for O II forbidden lines

Feb 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26a...173..410z&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 173, no. 2, Feb. 1987, p. 410-414.

Statistics

Computation

41

Forbidden Bands, Line Spectra, Oxygen Spectra, Radiative Transfer, Transition Probabilities, Atomic Energy Levels, Computational Astrophysics, Computer Programs, Magnetic Dipoles

Scientific paper

Following recent work by Butler and Zeippen (1984) on the forbidden lines between the 2p3 energy levels of neutral nitrogen, radiative transition probabilities have been calculated for O II forbidden lines, using the computer program SUPERSTRUCTURE. A configuration basis set has been selected, which yields satisfactory agreement with MCHF-BP calculations. The effect of semi-empirical term energy corrections and that of relativistic corrections to the magnetic dipole transition operator have been fully taken into account.

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