The C III problem

Details The C III problem The C III problem

Sep 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976a%26a....51..163l&link_type=abstract

Astronomy and Astrophysics, vol. 51, no. 2, Sept. 1976, p. 163-170.

Astronomy and Astrophysics

Astrophysics

33

Carbon, Electron Transitions, Emissivity, Fine Structure, Optical Transition, Quasars, Atomic Spectra, Beryllium, Line Spectra, Spectral Resolution, Transition Probabilities

Scientific paper

Various recently calculated emissivity ratios for C III transitions within the n 2 complex are examined in the light of intensities newly observed with better spectral resolution than in the past. Absolute and relative intensities were calculated from the transition region model of Gabriel (1976), but lack of agreement between certain intensity ratios found by different observers does not allow firm conclusions regarding its validity to be made.

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