Transition probabilities for N IV, O V, F VI, NE VII, and F V

Details Transition probabilities for N IV, O V, F VI, NE VII, and F V Transition probabilities for N IV, O V, F VI, NE VII, and F V

Apr 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979a%26a....74..244n&link_type=abstract

Astronomy and Astrophysics, vol. 74, no. 2, Apr. 1979, p. 244-246.

Astronomy and Astrophysics

Astrophysics

41

Atomic Energy Levels, Beryllium, Transition Probabilities, Fluorine, Neon, Nitrogen, Oxygen

Scientific paper

Transitions within the 2s(2)-2s2p-2p(2) configurations of the Be I sequence are among the best studied both theoretically and observationally. The paper presents calculated transition probabilities for four medium ionized members of the Be I sequence: N IV, O V, F VI, and Ne VII. Transition probabilities for F V are also calculated as an aid to the interpretation of F VI beam foil observations. The calculations are based on the microconfiguration method of Eissner et al. (1974). The study is an extension of the work of Nussbaumer and Storey (1978).

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