Hostname: page-component-78c5997874-94fs2 Total loading time: 0 Render date: 2024-11-05T16:56:37.769Z Has data issue: false hasContentIssue false
  • English
  • Français

Formation and maintenance of spiral structure in galaxies

Published online by Cambridge University Press:  04 August 2017

C. C. Lin  and
G. Bertin
C. C. Lin
Affiliation:
Massachusetts Institute of Technology Cambridge, MA. USA
G. Bertin
Affiliation:
Massachusetts Institute of Technology Cambridge, MA. USA

Abstract

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.

The formation and maintenance of spiral structure in galaxies is discussed in terms of spiral modes with a general perception consistent with the hypothesis of quasi-stationary spiral structure. The latter is explained in some detail to give it the original proper perspective and to contrast it with recent studies of non-stationary spiral structures. We again emphasize the possible coexistence of fast-evolving spiral features and slow-evolving spiral grand designs. Spiral modes are described in terms of three categories of propagating waves. The reason is given why isolated non-barred galaxies with spiral grand design are found to be mostly two-armed. Some suggestions are made for future research.

Type
PART III: Dynamics and Evolution
Information
Symposium - International Astronomical Union , Volume 106: The Milky Way Galaxy , 1985 , pp. 513 - 532
Copyright
Copyright © Reidel 1985 

References

Bertin, G.: 1980, Phys. Reports 61 (1), pp. 1–69 (217 references) Google Scholar
Bertin, G.: 1983a, Astron. Astrophys. 127, pp. 145–148 Google Scholar
Bertin, G.: 1983b, IAU Symposium No. 100, ed. Athanassoula, E. (Reidel), pp. 119–120 Google Scholar
Bertin, G. et al.: 1977, Proc. Nat. Acad. Sci. 74, pp. 4726–4729 CrossRefGoogle Scholar
Burton, W.B.: 1976, Ann. Rev. Astron. Astrophys. 14, pp. 275–306 Google Scholar
Burton, W.B., and Shane, W.W.: 1971, IAU Symposium 38, eds. Becker, W. and Contopoulos, G. (Reidel), pp. 397–414 Google Scholar
Dawson, J.M.: 1983, Rev. Modern Phys. 55, pp. 403–447 CrossRefGoogle Scholar
Drury, L. O'C.: 1980, Monthly Notices Roy. Astron. Soc. 193, pp. 337–343 Google Scholar
Goldreich, P., and Lynden-Bell, D.: 1965, Monthly Notices Roy. Astron. Soc. 130, 97, pp. 125 Google Scholar
Goldreich, P., and Tremaine, S.: 1978, Ap. J. 222, pp. 850–858 Google Scholar
Haass, J.: 1983a, in ‘Kinematics, Dynamics and Structure of the Milky Way’, ed. Shuter, W.L.H. (Reidel), pp. 283–287 Google Scholar
Haass, J.: 1983b, IAU Symposium No. 100, ed. Athanassoula, E. (Reidel), pp. 121–124 Google Scholar
Haass, J., Bertin, G., and Lin, C.C.: 1982, Proc. Nat. Acad. Sci. USA 79, pp. 3908–3912 Google Scholar
Iye, M., Okamura, S., Hamabe, M., and Watanabe, M.: 1982, Astrophys. J. 256, pp. 103–111 Google Scholar
Lau, Y.Y., and Bertin, G.: 1978, Ap. J. 226, pp. 508–520 Google Scholar
Lin, C.C.: 1971, in ‘Highlights of Astronomy’, ed. de Jager, C. (International Astron. Union, Reidel, Dordrecht, Netherlands), Vol. 2, pp. 88–121 Google Scholar
Lin, C.C.: 1983a, in ‘Kinematics, Dynamics and Structure of the Milky Way’, ed. Shuter, W.L.H. (Reidel), pp. 277–281 CrossRefGoogle Scholar
Lin, C.C.: 1983b, IAU Symposium No. 100, ed. Athanassoula, E. (Reidel), pp. 117–118 Google Scholar
Lin, C.C., and Bertin, G.: 1981, in ‘Plasma Astrophysics’, eds. Guyenne, T.D. and Levy, G. (European Space Agency, Noordwijk, Netherlands), SP-161, pp. 191–205 Google Scholar
Lin, C.C., and Lau, Y.Y.: 1979, Studies in Appl. Math. 60, pp. 97–163 Google Scholar
Lin, C.C., and Shu, F.H.: 1966, Proc. Nat. Acad. Sci. 55, pp. 229–234 Google Scholar
Lin, C.C., and Shu, F.H.: 1967, IAU Symposium No. 31, ed. van Woerden, H. (Academic Press, London), pp. 313–317 Google Scholar
Lin, C.C., and Yuan, C.: 1978, ‘Astronomical Papers dedicated to Bengt Strömgren’, eds. Reiz, A. and Andersen, T., published by Copenhagen University Observatory, pp. 369–386 Google Scholar
Lindblad, B.: 1963, Stockholm Observ. Ann. 22, No. 5 Google Scholar
Mark, J.W.-K.: 1976, Astrophys. J. 205, pp. 363–378 Google Scholar
Norman, C.: 1983, IAU Symposium No. 100, ed. Athanassoula, E. (Reidel), pp. 163–174 Google Scholar
Oort, J.: 1962, in ‘Interstellar Matter in Galaxies’, ed. Woltjer, L. (Benjamin, New York), pp. 234–244 Google Scholar
Roberts, W.W., Huntley, J.M., and van Albada, G.D.: 1979, Astrophys. J. 233, pp. 67–84 Google Scholar
Roberts, W.W., Roberts, M.S., and Shu, F.H.: 1975, Astrophys. J. 196, pp. 381–405 Google Scholar
Shu, F.H.: 1968, Ph. D. Dissertation, Harvard University Google Scholar
Shu, F.H., Milione, V., and Roberts, W.W.: 1973, Astrophys. J. 183, pp. 819–841 Google Scholar
Toomre, A.: 1969, Astrophys. J. 158, pp. 899–913 CrossRefGoogle Scholar
Toomre, A.: 1977, Ann. Rev. Astron. Astrophys. 15, pp. 437–478 Google Scholar
Toomre, A.: 1981, in ‘Structure and Evolution of Normal Galaxies’, eds. Fall, S.M. and Lynden-Bell, D. (Cambridge University Press), pp. 111–136 Google Scholar
Tremaine, S.: 1083, IAU Symposium No. 100, ed. Athanassoula, E. (Reidel), pp. 411–416 Google Scholar
Visser, H.C.D.: 1978, The dynamics of the spiral galaxy M81. Ph. D. thesis, University of Groningen, Netherlands Google Scholar
Van Dyke, M.: 1982, An Album of Fluid Motion (The Parabolic Press)Google Scholar