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Extended Atmospheres of Planetary Nuclei
Published online by Cambridge University Press: 08 February 2017
Abstract
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Exploratory calculations on nongray, hydrostatic-equilibrium model envelopes for central stars of planetary nebulae of high temperature and possibly near the instability limit are reported. It is conjectured that these may be related to Wolf-Rayet type nuclei; it appears possible to obtain an OV absorption, and OVI emission, spectrum even in an LTE calculation.
- Type
- Part A. Type of Problems that Exist
- Information
- International Astronomical Union Colloquium , Volume 2: Spectrum Formation in Stars With Steady-State Extended Atmospheres , August 1970 , pp. 54 - 60
- Copyright
- Copyright © 1970
References
Böhm, K. H.
1968, I.A.U. Symposium No. 34 “Planetary Nebulae,” eds. Osterbrock, D. R. and O'Dell, C. R., Dordrecht: D. Reidel Publ. Co., p. 297.Google Scholar
Carlson, B. G., and Lathrop, K. D.
1968, Computing Methods in Reactor Physics, eds. Greenspan, H., Kelber, C. N., Okrent, D., New York: Gordon and Breach, p. 167.Google Scholar
O'Dell, C. R.
1968, I.A.U. Symposium No. 34 “Planetary Nebulae,” eds. Osterbrock, D. E. and O'Dell, C. R., Dordrecht: D. Reidel Publ. Co., p. 361.Google Scholar
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