Appearance of lines of 'shaded' energy levels in spectra of planetary nebulae

Details Appearance of lines of 'shaded' energy levels in spectra of planetary nebulae Appearance of lines of 'shaded' energy levels in spectra of planetary nebulae

Jul 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980velen......111n&link_type=abstract

Leningradskii Universitet, Vestnik, Matematika, Mekhanika, Astronomiia, July 1980, p. 111-114. In Russian.

Astronomy and Astrophysics

Astronomy

Astronomical Spectroscopy, Energy Levels, Line Spectra, Planetary Nebulae, Radiative Recombination

Scientific paper

It is shown that the appearance of certain C III and N III lines associated with the shaded levels 2pnl(1, 3)L and 2s2p(3P)nl(2, 4)L can be explained in the framework of the recombination mechanism with allowance for interconfiguration transitions. It is shown that it is possible to construct total C III and N III spectra with both shaded and normal levels in planetary nebulae.

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