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A Possibility of Reveal of Parent Populations for the Objects by Active Nuclei on the Basis of Comparing their Spatial Correlation Functions

Published online by Cambridge University Press:  19 July 2016

B.V. Romberg  and
A.V. Kravtsov
B.V. Romberg
Affiliation:
Astrospace Center, Lebedev's Physical Institute, Profsoyuznaya St, 84/32, Moscow, 117810, Russia
A.V. Kravtsov
Affiliation:
Sternberg Astronomical Institute, Moscow State University, Universitetsky Pr, 13, Moscow, 117234, Russia

Extract

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For a model of the World with q 0 = 0.5 and H 0 = 100h −1 there was received a 2-point spatial correlation function (CF) (The sample of 300 objects with z < 0.045 and δ > 0 was used) for Seyfert Galaxies with the following parameters: r 0 = (9 ± 2)h −1 Mpc, γ = –(1.7 ± 0.2).

Type
Poster contributions: Statistical Studies and Evolution
Information
Symposium - International Astronomical Union , Volume 159: Multi-Wavelength Continuum Emission of AGN , 1994 , pp. 512
Copyright
Copyright © Kluwer 1994 

References

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2. Veron-Cetty, M.-P., and Veron, P. (1991). ESO Sci. Rep. No.10.Google Scholar
3. Shaver, P.A. (1984). Astron. Astrophys. 136, L9.Google Scholar