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The Absorption of Hell Lyα Photons in Planetary Nebulae

Published online by Cambridge University Press:  22 September 2016

D.R. Flower
Affiliation:
Observatoire de Meudon, Paris
M. Perinotto
Affiliation:
Astrofisico di Arcetri, Firenze

Extract

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The fate of the Hell Lya photons, produced during recombinations of the He++ ions and electrons, is important in considerations of the ionization and thermal structure of high excitation nebulae (Flower, 1968, IAU Symp. No. 34, Planetary Nebulae, p. 77). Hummer and Seaton (1964, M.N.R.A.S. 127, 217) effectively supposed that these photons are absorbed by H° in the central (He++) zone, whereas detailed line transfer calculations (Weymann and Williams, 1969, Ap. J. 157, 1201; Harrington, 1972, Ap. J. 176, 127) suggest that a large fraction of the photons escapes from the central zone. We consider the effects of the absorption of these photons on the ionization and thermal structure of the outer (He+, H+) zone of a nebula which is optically thick in the HI Lyman continuum. (Paper will appear in Astronomy and Astrophysics.)

Type
Session III: Physical Processes
Copyright
Copyright © Reidel 1978