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The correlation function of galaxies in the direction of the Coma cluster

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Abstract

The observational data on the amplitude of the correlation function of galaxies in the direction of the Coma cluster are confronted with an analytic formula derived for a self-similar observer-homogeneous structure.

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References

  • Calzetti, D., Giavalisco, M., Pietronero, L., and Ruffini, R.: 1987a,Phys. Rev. Letters (submitted).

  • Calzetti, D., Giavalisco, M., and Ruffini, R.: 1987b,Astron. Astrophys. (submitted).

  • Einasto, J., Klypin, A. A., and Saar, E.: 1986,Monthy Notices Roy. Astron. Soc. 219, 457.

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  • Ruffini, R., Song, D. J., and Taraglio, S.: 1987,Astron. Astrophys. (in press).

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Authors and Affiliations

  1. I.C.R.A., International Center for Relativistic Astrophysics, Dip. di Fisica, Università di Roma ‘La Spapienza’, Italy

    D. Calzetti, M. Giavalisco & R. Ruffini

  2. Tartu Astrophysical Observatory, Toravere, Estonia, U.S.S.R.

    J. Einasto & E. Saar

Authors
  1. D. Calzetti
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  2. J. Einasto
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  3. M. Giavalisco
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  4. R. Ruffini
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  5. E. Saar
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Calzetti, D., Einasto, J., Giavalisco, M. et al. The correlation function of galaxies in the direction of the Coma cluster. Astrophys Space Sci 137, 101–106 (1987). https://doi.org/10.1007/BF00641624

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  • DOI: https://doi.org/10.1007/BF00641624

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