• The O III 52 ▪m/88 ▪m emission-line ratio in planetary nebulae

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    • Keywords


      emission-line diagnostics; electron densities; planetary nebulae

    • Abstract


      R-matrix calculations of electron impact excitation rates in 0 III are used to derive the electron-density-sensitive emission-line ratioR = 1 (2s2 2p23P2-2s22P23P1)/I (2s22p23P1 - 2s22p23P0) =I (52μm)/I (88μm) for a range of electron temperatures(Te = 5000-20000 K) and densities(Ne=10–105 cm−3) applicable to planetary nebulae. Electron densities deduced from the observed values ofR in several planetary nebulae are in excellent agreement with those deduced from C1 I and Ar IV, which provides support for the accuracy of the atomic data adopted in the calculations.

    • Author Affiliations


      F. P. Keenan1 K. M. Aggarwal2

      1. Department of Pure and Applied Physics, Queen’s University of Belfast, Belfast - BT7 1NN, N. Ireland
      2. Department of Physics and Astrophysics, University of Delhi, Delhi - 110007
    • Dates

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