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Abstract

An exhaustive study of QSO galaxy associations in a given sky region (Arp) shows an anomalous distribution: the histogram of the associations as a function of their "probability" p has a strong maximum for p +- 10**-2, very different from what is expected from an uncorrelated distribution.

Additional information

Authors: DUBOIS M A, CEA, FONTENAY-AUX-ROSES (FRANCE);LABORATOIRE DE PHYSIQUE THEORIQUE, PARIS (FRANCE);GIRAUD E, CEA, FONTENAY-AUX-ROSES (FRANCE);LABORATOIRE DE PHYSIQUE THEORIQUE, PARIS (FRANCE);VIGIER J P CEA, FONTENAY-AUX-ROSES (FRANCE), CEA, FONTENAY-AUX-ROSES (FRANCE);LABORATOIRE DE PHYSIQUE THEORIQUE, PARIS (FRANCE);LABORATOIRE DE PHYSIQUE THEORIQUE, PARIS (FRANCE), CEA, FONTENAY-AUX-ROSES (FRANCE);LABORATOIRE DE PHYSIQUE THEORIQUE, PARIS (FRANCE)
Bibliographic Reference: C.R. ACAD. SC. PARIS, VOL. 297 (1983), SERIES II, PP. 259-260
Record Number: 1989122048400 / Last updated on: 1987-01-01
Category: PUBLICATION
Available languages: en
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