O III - Intercombination and forbidden lines

Details O III - Intercombination and forbidden lines O III - Intercombination and forbidden lines

Jun 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26a....99..177n&link_type=abstract

Astronomy and Astrophysics, vol. 99, no. 1, June 1981, p. 177-181.

Astronomy and Astrophysics

Astrophysics

131

Astronomical Spectroscopy, Forbidden Transitions, Nebulae, Oxygen Ions, Radiative Transfer, Transition Probabilities, Atomic Energy Levels, Electron States, Fine Structure, Particle Interactions, Population Theory, Quasars, Stellar Spectra

Scientific paper

We calculate radiative transition probabilities in 0111, in particular for the intercombination transitions 2s22p2 3P - 2s2p3 5S0. We derive relative populations for the 6 lowest levels in O2+ for conditions found in gaseous nebulae, symbiotic stars and QSO. Attention is drawn to the interpretational value of the multiplets at λλ166l, 1667, and λ2322, as being complementary to the well known forbidden lines at λλ4363, 4960, 5008.

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