Hostname: page-component-cd9895bd7-gbm5v Total loading time: 0 Render date: 2024-12-13T02:26:53.976Z Has data issue: false hasContentIssue false
  • English
  • Français

Typical Scales in Distribution of IRAS Galaxies

Published online by Cambridge University Press:  25 May 2016

Z. G. Deng ,
X. Y. Xia  and
G. Börner
Z. G. Deng
Affiliation:
Dept. of Physics, Graduate School, USTC, P.R. China
X. Y. Xia
Affiliation:
Dept. of Physics, Tianjin Normal University, P.R. China
G. Börner
Affiliation:
Max-Planck-Institut für Astrophysik, D-85740, Germany

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.

Typical scales in the distribution of IRAS galaxies have been searched for with the unnormalized pair count method given by Mo et al.1. Samples consist of a) galaxies from QDOT with | b | ≥ 20°; b) galaxies from the IRAS faint source catalog(FSC) with f60 ≥ 0.3 Jy and | b | ≥ 30°. Galaxies with b ≥ 0 and b ≤ 0 were treated as independent samples in our analysis.

Type
IV. Structure Formation and Dark Matter
Information
Symposium - International Astronomical Union , Volume 183: Cosmological Parameters and the Evolution of the Universe , 1999 , pp. 246
Copyright
Copyright © Kluwer 1999 

References

1. Mo, H. J., Deng, Z. G., Xia, X. Y., Schiller, P. and Börner, G. (1992b) AA. 257, 1 Google Scholar
2. Mo, H. J., Xia, X. Y., Deng, Z. G., Börner, G. and Fang, L. Z. (1992a) AA, 256, L23 Google Scholar
3. Deng, Z. G., Xia, X. Y. and Fang, L. Z. (1994) ApJ, 431, 506 CrossRefGoogle Scholar