Publication Abstracts

Sofia and Hunter 1968

Sofia, S., and J.H. Hunter, Jr., 1968: Dynamical models of planetary nebulae. Astrophys. J., 152, 405-415, doi:10.1086/149557.

Dynamical models of spherically symmetric, optically thin planetary nebulae have been constructed utilizing an accurate numerical scheme and taking account of the thermal behavior of the gas in detail. The evolution of several model nebulae is exhibited and conclusions are drawn regarding some initial conditions that must prevail in the ejected shell.

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BibTeX Citation

  author={Sofia, S. and Hunter, Jr., J. H.},
  title={Dynamical models of planetary nebulae},
  journal={Astrophys. J.},

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RIS Citation

ID  - so04100j
AU  - Sofia, S.
AU  - Hunter, J. H., Jr.
PY  - 1968
TI  - Dynamical models of planetary nebulae
JA  - Astrophys. J.
VL  - 152
SP  - 405
EP  - 415
DO  - 10.1086/149557
ER  -

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