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Quasar evolution via dark halo merger

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Abstract

Imaging surveys indicate that galaxy interaction or merging plays an important role in triggering the quasar phenomenon. It is assumed that a luminous quasar is created in the center of a merger of virialized dark matter halos. The abundance and evolution of quasars are computed in the cold dark matter models. The comparison between observational data and model predictions is presented.

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References

  1. Shaver, P. A., Wall, J. V., Kellermann, K. L. et al., Decrease in the space density of quasars at high redshift,Nature, 1996, 384: 439.

    Article  Google Scholar 

  2. Efstathiou, G., Rees, M. J., High-redshift quasars in the cold dark matter cosmogony,MNRAS, 1988, 230: 5.

    Google Scholar 

  3. Nusser, A., Silk, J., Abundance and evolution of quasars in cold dark matter models,ApJ, 1993, 411: L1.

    Article  Google Scholar 

  4. Robson, I.,Active Galactic Nuclei, New York: John Wiley & Sons, 1996.

    Google Scholar 

  5. Toomre, A., inEvolution of Galaxies and Stellar Populations (eds. Tinsley, B. M., Larson, R. B.), New Haven: Yale Observatory, 1977.

    Google Scholar 

  6. Sanders, D. B., Soifer, B. T., Elias, J. H. et al., Warm ultraluminous galaxies in the IRAS survey: The transition from galaxy to quasars?,ApJ, 1988, 328: L35.

    Article  Google Scholar 

  7. Bahcall, J. N., Kirhakos, S., Saxe, D. H. et al., Hubble Space Telescope images of a sample of 20 nearby luminous quasars,ApJ, 1997, 479: 642.

    Article  Google Scholar 

  8. Bond, J. R., Efstathiou, G., Cosmic background radiation anisotropies in universe dominated by nonbaryonic dark matter,ApJ, 1984, 285: L45.

    Article  Google Scholar 

  9. Peebles, P. J. E.,Principles of Physical Cosmology, Newjersey: Princeton University Press, 1993.

    Google Scholar 

  10. Smoot, G. F., Bennett, C. L., Kogut, A. et al., Structure in the COBE DMR first-year maps,ApJ, 1992, 396: L1.

    Article  Google Scholar 

  11. Saslaw, W. C.,Gravitational Physics of Stellar and Galactic Systems, Cambridge: Cambridge University Press, 1985.

    Google Scholar 

  12. Carlberg, R. G., Quasars evolution via galaxy mergers,ApJ, 1990, 350: 505.

    Article  Google Scholar 

  13. Klypin, A., Holtzman, J., Primack, J. et al., Structure formation with cold plus hot dark matter,ApJ, 1993, 416: 1.

    Article  Google Scholar 

  14. Wilson, A. S., Colberg, E. J. M., The difference between radio-loud and radio-quiet active galaxies,ApJ, 1998, 438: 62.

    Article  Google Scholar 

  15. Kormendy, J., Richstone, D., Inward bound—The search for supermassive black holes in galactic nuclei,ARA & A, 1998, 33: 581.

    Google Scholar 

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Zhang, Y., Chu, Y. Quasar evolution via dark halo merger. Sci. China Ser. A-Math. 41, 330–336 (1998). https://doi.org/10.1007/BF02879053

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  • DOI: https://doi.org/10.1007/BF02879053

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