Hostname: page-component-586b7cd67f-gb8f7 Total loading time: 0 Render date: 2024-11-28T09:44:16.742Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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

1. Lipovetsky, V.A., et al. (1989). A Catalogue of galaxies Sy-types , SAO, USSR Google Scholar
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