No CrossRef data available.
Article contents
Comparison of Gas and Radiation Pressure in the Problems of the Dynamics of Planetary Nebulae
Published online by Cambridge University Press: 03 August 2017
Extract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
We may summarize Wilson's extended study of internal motions in planetary nebulae by stating that he finds the average expansion velocity in the regions whence originate the lines of H, NeIII, OIII to be roughly 20 km/sec, with rare examples ranging as low as O and as high as 50 km/sec. We ask whether radiation pressure and/or gas pressure may give, in an elementary calculation, velocities anywhere near these values.
- Type
- Part V: Kinematic Structure of Gaseous Envelopes
- Information
- Symposium - International Astronomical Union , Volume 8: Cosmical Gas Dynamics , July 1958 , pp. 1030 - 1033
- Copyright
- Copyright © American Physical Society 1958
References
1 Wilson, O. C., Astrophys. J. 111, 279 (1950).Google Scholar
2 Zanstra, H., Bull. Astron. Soc. Neth. 12, No. 465, 349 (1956).Google Scholar
3 Oort, J. H., Bull. Astron. Soc. Neth. 12, No. 455, 177 (1955).Google Scholar
4 Zanstra, H., Monthly Notices Roy. Astron. Soc. 93, 131 (1932).Google Scholar
5 Wurm, K., Contr. Obs. Astrof. U. di Padova in Asiage No. 73, p. 91 (1956).Google Scholar
6 Aller, L. H., Gaseous Nebulae (Chapman and Hall, London, 1956), pp. 56–57, Fig. III 5.Google Scholar
7 Minkowski, R., Gas Dynamics of Cosmic Clouds , edited by van de Hulst, H. C. and Burgers, J. M. (North Holland Publishing Company, Amsterdam, the Netherlands, 1955), pp. 11–12.Google Scholar
You have
Access