Astrophysics and Space Science

, Volume 14, Issue 1, pp 52–55 | Cite as

The hose-pipe instability in stellar systems

  • R. M. Kulsrud
  • James W. K. Mark
  • A. Caruso

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References

  1. Antonov, V. A.: 1960,Soviet Astron. 4, 859.Google Scholar
  2. Antonov, V. A.: 1962,J. Leningrad Univ. 7, 135 (available in translation Princeton Plasma Physics Laboratory Report PPL-Trans-1 (1969) 34 pp.).Google Scholar
  3. Ipser, J. R. and Thorne, K. S.: 1968,Astrophys. J. 154, 251.Google Scholar
  4. Kulsrud, R. M. and Mark, J. W. K.: 1960,Astrophys. J. 160, 471.Google Scholar
  5. Lynden Bell, D. and Sanitt, N.: 1969,Monthly Notices Roy. Astron. Soc. 143, 167.Google Scholar
  6. Milder, D. M.: 1969, ‘Rotating Stellar Systems’, unpubl. Ph.D. thesis, Harvard Univ.Google Scholar
  7. Toomre, A.: 1966, ‘A Kelvin-Helmholtz Instability’, Notes from the Geophysical Fluid Dynamics Summer Program, Woods Hole Oceanographic Inst., pp. 111–114.Google Scholar

Copyright information

© D. Reidel Publishing Company 1971

Authors and Affiliations

  • R. M. Kulsrud
    • 1
  • James W. K. Mark
    • 1
  • A. Caruso
    • 2
  1. 1.Plasma Physics LaboratoryPrinceton UniversityPrinceton
  2. 2.Laboratori Gas IonizzatiFrascatiItaly
  3. 3.Mathematics DepartmentMassachusetts Institute of TechnologyCambridge

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