Skip to main content
SpringerLink
Log in

On the origin of tightly wound spiral features in galactic nuclei

  • Published:
Astrophysics Aims and scope

This is a preview of subscription content, log in via an institution to check access.

Access this article

Log in via an institution

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Institutional subscriptions

Literature Cited

  1. J. L. Sersic, Pastoriza, P. A. S. P.,77, 287 (1965).

    Google Scholar 

  2. M. F. Walker, Astrophys. J.,151, 71 (1968).

    Google Scholar 

  3. M. F. Walker, Astrophys. J.,73, 854 (1968).

    Google Scholar 

  4. M. H. Ulrich, Astrophys. J.,181, 54 (1973).

    Google Scholar 

  5. G. Courtes, C.R. Acad. Sci.253, 218 (1961).

    Google Scholar 

  6. P. C. van der Kruit, J. H. Oort, and D. S. Mathewson, Astron. Astrophys.,21, 169 (1972).

    Google Scholar 

  7. W. K. Ford and V. C. Rubin, Bull. AAS,2, 192 (1970).

    Google Scholar 

  8. S. T. Gottesman, R. Lucas, L. Waliachew, and M. C. H. Wright, Astrophys. J.,204, 699 (1976).

    Google Scholar 

  9. M. H. Ulrich, Astrophys. J.,219, 424 (1978).

    Google Scholar 

  10. P. C. van der Kruit, Astrophys. J.,188, 3 (1974).

    Google Scholar 

  11. S. M. Simkin, Astrophys. J.,195, 293 (1977).

    Google Scholar 

  12. V. C. Rubin, W. K. Ford, and C. J. Peterson, Astrophys. J.,199, 39 (1975).

    Google Scholar 

  13. V. C. Rubin, N. Thonnard, and W. K. Ford, Astrophys. J. Lett.,217, L1 (1977).

    Google Scholar 

  14. M. F. Duval, Astrophys. Space Sci.,48, 103 (1977).

    Google Scholar 

  15. V. C. Rubin, N. Thonnard, and W. K. Ford, Astrophys. J.,199, 31 (1975).

    Google Scholar 

  16. P. Pismis, Bol. Obs. Tonantzintla y Tacubaya,19, 7 (1960).

    Google Scholar 

  17. S. S. Huang and P. Pismis, Bol. Obs. Tonantzintla y Tacubaya,19, 7 (1960).

    Google Scholar 

  18. V. A. Ambartsumian, La Structure of l'Evolution de l'Univers, Stoops, Bruxelles (1958), p. 241.

    Google Scholar 

  19. P. Pismis, Bol. Obs. Tonantzintla y Tacubaya,3, 3 (1961).

    Google Scholar 

  20. P. Pismis, Bol. Obs. Tonantzintla y Tacubaya,3, 119 (1963).

    Google Scholar 

  21. P. Pismis, The Large-Scale Characteristics of the Galaxy, IAU Symposium, No. 84 (ed. W. B. Burton), Reidel (1979), p. 145.

  22. R. Wielen, The Large-Scale Characteristics of the Galaxy, IAU Symposium No. 84 (ed. (W. B. Burton), Reidel (1979), p. 183.

  23. P. C. van der Kruit, Astron. Astrophys.,52, 85 (1976).

    Google Scholar 

Download references

Authors
  1. P. Pismis
    View author publications

    You can also search for this author in PubMed Google Scholar

  2. E. Moreno
    View author publications

    You can also search for this author in PubMed Google Scholar

Additional information

Instituto de Astronomia, Universidad Nacional Autonoma de Mexico. Published in English in Astrofizika, Vol. 20, No. 1, pp. 7–20, January–February, 1984, and republished here with minor editorial modifications.

Rights and permissions

Reprints and permissions

About this article

Cite this article

Pismis, P., Moreno, E. On the origin of tightly wound spiral features in galactic nuclei. Astrophysics 20, 1–10 (1984). https://doi.org/10.1007/BF01005894

Download citation

  • Received:

  • Accepted:

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF01005894

Keywords

Search

Navigation