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On the Generation of the Hubble Sequence Through an Internal Secular Dynamical Process

  • Xiaolei Zhang
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 319)

Abstract

The secular evolution process, which slowly transforms the morphology of a galaxy over its lifetime, could naturally account for observed properties of the great majority of physical galaxies if both stellar and gaseous accretion processes are taken into account. As an emerging paradigm for galaxy evolution, its dynamical foundation had been established in the past few years, and its observational consequences are yet to be fully explored. The secular evolution picture provides a coherent framework for understanding the extraordinary regularity and the systematic variation of galaxy properties along the Hubble sequence.

Keywords

Generation of the Hubble Sequence Secular evolution of galaxies 

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References

  1. Andredakis, YC, Peletier, R.F., and Balcells, M. 1995, MNRAS, 275, 874ADSGoogle Scholar
  2. Binney, J., and Tremaine, S. 1987, Galactic Dynamics (Princeton:Princeton Univ. Press)Google Scholar
  3. Bell, E.F. and de Jong, R.S. 2001, ApJ, 550, 212.ADSCrossRefGoogle Scholar
  4. Combes, F., and Sanders, R.H. 1981, AandA, 96, 164Google Scholar
  5. Conselice, C.J., Kershady, M.A., Dickinson, M., and Papovich, C. 2003, AJ, 126, 1183ADSCrossRefGoogle Scholar
  6. de Blok, W.J.G. 2003, presented in Dark Matter in Galaxies, IAUS 220Google Scholar
  7. Djorgovski, S. and Davis, M. 1987, ApJ, 313, 59ADSCrossRefGoogle Scholar
  8. Dressler, A. et al. 1987, ApJ, 313, 42ADSCrossRefGoogle Scholar
  9. Faber, S.M., et al. in Nearly Normal Galaxies, ed. S.M. Faber ( New York: Springer ), 175Google Scholar
  10. Faber, S.M., and Jackson, R.E. 1976, ApJ, 204, 668ADSCrossRefGoogle Scholar
  11. Freeman, K.C. 1970, ApJ, 160, 811ADSCrossRefGoogle Scholar
  12. Hamabe, M., and Kormendy, J. 1987, in Structure and Dynamics of Elliptical Galaxies, ed T. de Zeeuw (lAU), 379Google Scholar
  13. Jablonka, P., Gorgas, J., and Goudfrooij, P. 2002, ApandSS, 281, 367Google Scholar
  14. Kormendy, J. 1982, in 12th Advanced Course of the SSAA, eds. L. Martinet, and M. Mayor ( Geneva Observatory: Geneva ), 115Google Scholar
  15. Kormendy, J., and Kennicutt, R. 2004, ARAandA, in pressGoogle Scholar
  16. Lynden-Bell, D., and Kalnajs, A.J., 1972, MNRAS, 157, 1ADSGoogle Scholar
  17. McGaugh, S.S., and de Blok, W.J.G. 1998, ApJ, 499, 41ADSCrossRefGoogle Scholar
  18. Peebles, J. 1983, Physical Cosmology (Princeton: Princeton Univ. Press)Google Scholar
  19. Persic, M., Salucci, P., and Stel, F. 1996, MNRAS, 281, 27ADSGoogle Scholar
  20. Pharasyn, A., Simien, F., and Heraudeau, Ph. 1997, in Dark and Visible Matter in Galaxies, ASP Conf. Series 117, eds M. Persic and P Salucci ( San Francisco: ASP ), 180Google Scholar
  21. Shu, F.S., 1982, The Physical Universe: An Introduction to Astronomy ( Mill Valley: University Science Books )Google Scholar
  22. Toomre, A., and Toomre, J. 1972, ApJ, 178, 623ADSCrossRefGoogle Scholar
  23. Tully, R.B., and Fisher, J.R. 1977, AandA, 54, 661Google Scholar
  24. Wielen, R. 1977, AandA, 60, 263Google Scholar
  25. Wolfe, A.M., 2001, in Galaxy Disks and Disk Galaxies, eds J.G. Funes, S.J. and E.M. Corsini ( San Francisco: ASP ), 619Google Scholar
  26. Zhang, X. 1996, ApJ, 457, 125; 1998, ApJ, 499, 93; 1999, ApJ, 518, 613ADSGoogle Scholar
  27. Zhang, X., 2002, ApandSS, 281, 281Google Scholar
  28. Zhang, X. 2003, JKAS, 36, 223ADSGoogle Scholar
  29. Zhang, X., Lee, Y., Bolatto, A., and Stark, A.A., 2001, ApJ, 553, 274ADSCrossRefGoogle Scholar
  30. Zwaan, M.A., van der Hulst, J.M., de Bolk, W.J.G., and McGaugh, S.S. 1995, MNRAS, 273, L35ADSGoogle Scholar

Copyright information

© Springer Science+Business Media New York 2004

Authors and Affiliations

  • Xiaolei Zhang
    • 1
  1. 1.US Naval Research LaboratoryUSA

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