Hostname: page-component-cd9895bd7-lnqnp Total loading time: 0 Render date: 2024-12-12T19:50:32.657Z Has data issue: false hasContentIssue false
  • English
  • Français

Theoretical considerations of the warp and thickening

Published online by Cambridge University Press:  14 August 2015

E. Saar
E. Saar*
Affiliation:
Tartu Astrophysical Observatory

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.

As a theoretical subject, the study of the bending of the gaseous planes of galaxies has not been extremely popular. It seems that this is due to an excellent and thorough paper on the subject, published by Hunter and Toomre in 1969. At that time there existed three (or four) rival theoretical mechanisms:

  1. (1) vertical oscillations of the galactic disk, considered first by Lynden-Bell (1965);

  2. (2) asymmetrical pressure on the disk due to intergalactic wind (Kahn and Woltjer 1959);

  3. (3) tidal influence of the Magellanic Clouds, from

    1. (a) the case of Stationary Clouds, and

    2. (b) the case of Clouds orbiting around the Galaxy (Elwert and Hablick 1965, Avner and King 1967).

Type
IX. THE GALACTIC WARP
Information
Symposium - International Astronomical Union , Volume 84: The Large-Scale Characteristics of the Galaxy , 1979 , pp. 513 - 522
Copyright
Copyright © Reidel 1979 

References

Aarseth, S. J. and Binney, J: 1978, preprint.Google Scholar
Avner, E. S., and King, I. R.: 1967, Astron. J. 72, 650.Google Scholar
Binney, J.: 1977, preprint.Google Scholar
Burke, B. G.: 1957, Astron. J. 62, 90.Google Scholar
Doroshkevich, A. G., Sunyaev, R. A., and Zeldovich, Ya.B.: 1974, in Longair, M. S. (ed.) Confrontation of Cosmological Theories with Observational Data, IAU Symp. 63, 213.Google Scholar
Einasto, J., Joêveer, M., and Kaasik, A.: 1976, Tartu Astrophys. Obs. Teated No. 54, 3.Google Scholar
Elwert, G., and Hablick, D.: 1965, Z. Astrophys. 61, 273.Google Scholar
Fujimoto, M., and Sofue, Y.: 1976, Astron. Astrophys. 47, 263.Google Scholar
Fujimoto, M., and Sofue, Y.: 1977, Astron. Astrophys. 61, 199.Google Scholar
Gunn, J. E.: 1977, in Tinsley, B. M. and Larson, R. B. (eds.). The Evolution of Galaxies and Stellar Populations, Yale University Observatory, 445.Google Scholar
Haud, U.: 1977, .Google Scholar
Hunter, C.: 1969, Stud. Appl. Math. 48, 55.Google Scholar
Hunter, C., and Toomre, A.: 1969, Astrophys. J. 155, 747.Google Scholar
Jaaniste, J.: 1977, .Google Scholar
Jaaniste, J., and Saar, E.: 1976, Tartu Astrophys. Obs. Teated No. 54, 93.Google Scholar
Kahn, F. D., and Woltjer, L.: 1959, Astrophys. J. 130, 705.CrossRefGoogle Scholar
Kerr, F. J.: 1957, Astron. J. 62, 93.CrossRefGoogle Scholar
Lynden-Bell, D.: Monthly Notices Roy. Astron. Soc. 129, 299.Google Scholar
McKee, C. F., and Ostriker, J. P.: 1977, preprint.Google Scholar
Polyachenko, V. L., and Fridman, A. M.: 1976, The Equilibrium and Stability of Gravitating Systems, Moscow.Google Scholar
Sancisi, R.: 1976, Astron. Astrophys. 53, 159.Google Scholar
Shapiro, P. R., and Field, G. B.: 1976, Astrophys. J. 205, 762.CrossRefGoogle Scholar
Spight, L., and Grayzeck, E.: 1977, Astrophys. J. 213, 374.Google Scholar
Toomre, A.: 1970, in the Spiral Structure of our Galaxy.Google Scholar