Transition probabilities for forbidden lines in the 2p/3/ configuration

Details Transition probabilities for forbidden lines in the 2p/3/ configuration Transition probabilities for forbidden lines in the 2p/3/ configuration

Jan 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982mnras.198..111z&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 198, Jan. 1982, p. 111-125.

Astronomy and Astrophysics

Astrophysics

132

Forbidden Transitions, Ground State, Isoelectronic Sequence, Nebulae, Nitrogen Ions, Transition Probabilities, Astrophysics, Atomic Structure, Magnetic Dipoles, Radiative Transfer, Spin-Orbit Interactions

Scientific paper

Making use of the atomic structure computer program SUPERSTRUCTURE, radiative transition probabilities are calculated for the forbidden lines in the ground configuration 1s(2)2s(2)2p(3) of all the members of the isoelectronic sequence from N I to Fe XX. Elaborate procedures, such as configuration interaction, semi-empirical term energy corrections, special radial wave functions and relativistic corrections to the magnetic dipole operator, are used in the present calculation. This results in improvements over previous work. The importance of such changes is discussed with regard to some astrophysical problems

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