Skip to main content

Phenomenology of Spiral Galaxies

  • Chapter
Structure and Evolution of Galaxies

Part of the book series: NATO Advanced Study Institutes Series ((ASIC,volume 21))

Abstract

Galaxies have probably been formed from fluctuations in density and motion in the universe. Many cosmologists have suggested that the separation into individual units took place around the time of decoupling of matter and radiation, when the radius of the universe was about 1/1000th of the present radius. In this case the protogalaxies must have obtained their angular momentum at a later stage in their evolution, through interaction with other protogalaxies or with galaxy clusters. For when the radius of the universe was 1/1000th of its present value, and the density about 10−20g cm−3, a mass of, say, 1011M would have had a radius of 10 cm. A mass with such a radius cannot contain anything like the angular momentum contained in a galaxy like the Milky Way system.

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

Access this chapter

Chapter
USD 29.95
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
eBook
USD 39.99
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
Softcover Book
USD 54.99
Price excludes VAT (USA)
  • Compact, lightweight edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info

Tax calculation will be finalised at checkout

Purchases are for personal use only

Institutional subscriptions

Preview

Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.

References

  1. J.P. Ostriker and P.J.E. Peebles, Astrophys.J. 186, 467, 1973.

    Google Scholar 

  2. Stellar Populations, ed. D.J.K, O’Connell, North-Holland Publ. Co., 1958.

    Google Scholar 

  3. Alan Sandage, The Hubble Atlas of Galaxies, Carnegie Inst. of Washington 1961. Publication 618.

    Google Scholar 

  4. W.W. Morgan, Publ.Astr.Soc.Pacific 70, 364, 1958, and Spiral Structure in External Galaxies, in: I.A.U. Symposium No. 38, The Spiral Structure of our Galaxy, Ed. W.Becker and G. Contopoulos, D. Reidel Publ. Co., Dordrecht, Holland, 1970.

    Article  ADS  Google Scholar 

  5. W.W. Morgan and N.U. Mayall, Publ.Astr.Soc.Pacific 69, 291, 1957.

    Article  ADS  Google Scholar 

  6. G. and A. de Vaucouleurs, Reference Catalogue of Bright Galaxies, Univ. of Texas Press, Austin, 1964.

    Google Scholar 

  7. C.J. van Houten, Bull.Astr.Inst.Netherlands 16, 1, 1961.

    ADS  Google Scholar 

  8. W. Baade and L. Spitzer, Astrophys. J. 113, 413, 1951.

    Article  ADS  Google Scholar 

  9. D.S. Mathewson, P.C. van der Kruit and W. Brouw, Astron.Astrophys. 17, 468, 1972.

    ADS  Google Scholar 

  10. A.H. Rots and W.W. Shane, Astron. Astrophys. 31, 245, 1974.

    ADS  Google Scholar 

  11. C. Balkowski, Astron. Astrophys. 29, 43, 1973.

    ADS  Google Scholar 

  12. L. Bottinelli, Astron.Astrophys. 10, 437, 1971.

    ADS  Google Scholar 

  13. A.H. Rots, Distribution and Kinematics of Neutral Hydrogen in the Spiral Galaxy M81, Doctor’s thesis, Groningen, 1974.

    Google Scholar 

  14. J.H. Oort, Astron. Astrophys. 7, 381, 1970.

    ADS  Google Scholar 

  15. A comprehensive survey has been given by A.M. Hulsbosch, Doctor’s thesis, Leiden, 1972.

    Google Scholar 

  16. R.D. Davies, Nature 237, 88, 1972.

    Article  ADS  Google Scholar 

  17. G.L. Verschuur, Astron. Astrophys. 22, 139, 1973.

    ADS  Google Scholar 

  18. G.W. Rougoor and J.H. Oort, Proc.Nat.Ac.Washington, D.C. 46, 1, 1960.

    Article  ADS  Google Scholar 

  19. P.C. van der Kruit, Astron.Astrophys. 13, 405, 1971.

    ADS  Google Scholar 

  20. S.C. Simonson III and G.L. Mader, Astron. Astrophys. 27, 337, 1973.

    ADS  Google Scholar 

  21. G.W. Rougoor, Bull.Astr.Inst.Netherlands 17, 381, 1964.

    ADS  Google Scholar 

  22. J.H. Oort, in Les Noyaux des Galaxies, ed.D.J.K. O’Connell, Pontif. Ac.Sc. Scripta Varia 35, 1971.

    Google Scholar 

  23. R.H. Sanders and G.T. Wrixon, Astron. Astrophys. 26, 365, 1973.

    ADS  Google Scholar 

  24. R.H. Sanders and T. Lowinger, Astron. J. 77, 292, 1972.

    Article  ADS  Google Scholar 

  25. Aa. Sandqvist, Astron. J. 75, 135, 1970.

    Article  ADS  Google Scholar 

  26. E.E. Becklin and G. Neugebauer, Astrophys. J. 151, 145, 1968.

    Article  ADS  Google Scholar 

  27. G.H. Rieke and F.J. Low, Astrophys. J. 184, 415, 1973.

    Article  ADS  Google Scholar 

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

    ADS  Google Scholar 

  29. G. Courtès and P. Cruvellier, C.R. Acad.Sci. Paris 253, 218, 1961.

    Google Scholar 

  30. G. Courtes, M. Viton and P. Vèron in Quasi-Stellar Sources and Gravitational Collapse, ed. Robinson et al, Univ. of Chicago Press, Chicago, III. 1965.

    Google Scholar 

  31. P.C. van der Kruit, Astrophys. J., 192, 1, 1974.

    Article  ADS  Google Scholar 

  32. B. Balick and R.L. Brown, Astrophys.J. 194, in print, 1974.

    Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Editor information

Editors and Affiliations

Rights and permissions

Reprints and permissions

Copyright information

© 1975 D. Reidel Publishing Company, Dordrecht, Holland

About this chapter

Cite this chapter

Oort, J.H. (1975). Phenomenology of Spiral Galaxies. In: Setti, G. (eds) Structure and Evolution of Galaxies. NATO Advanced Study Institutes Series, vol 21. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-1718-3_6

Download citation

  • DOI: https://doi.org/10.1007/978-94-010-1718-3_6

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-1720-6

  • Online ISBN: 978-94-010-1718-3

  • eBook Packages: Springer Book Archive

Publish with us

Policies and ethics