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Astrophysics and Space Science

, Volume 18, Issue 1, pp 223–225 | Cite as

The floccule theory for planetary formation

  • I. P. Williams
Article

Abstract

The accumulation of floccules into protoplanets is discussed, and it is pointed out that the simplifications which have been introduced into recent numerical models may result in the incorrect conclusion being reached.

Keywords

Numerical Model Incorrect Conclusion Planetary Formation Recent Numerical Model 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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References

  1. Aust, C. and Woolfson, M. M.: 1971,Monthly Notices Roy. Astron. Soc. 153, 21P.Google Scholar
  2. McCrea, W. H.: 1960,Proc. Roy. Soc. A256, 245.Google Scholar
  3. Williams, I. P.: 1969,Monthly Notices Roy. Astron. Soc. 146, 339.Google Scholar
  4. Williams, I. P. and Galley, S. J.: 1971,Monthly Notices Roy. Astron. Soc. 151, 207.Google Scholar
  5. Woolfson, M. M.: 1969,Prog. Phys. 32, 135.Google Scholar

Copyright information

© D. Reidel Publishing Company 1972

Authors and Affiliations

  • I. P. Williams
    • 1
  1. 1.Applied Mathematics DepartmentQueen Mary CollegeLondonEngland

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