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Observational Evidence for Non-Velocity Redshift in Stephan's Quintet

Published online by Cambridge University Press:  14 August 2015

C. Balkowski ,
L. Bottinelli ,
P. Chamaraux ,
L. Gouguenheim  and
J. Heidmann
C. Balkowski
Affiliation:
Observatoire de Paris, Meudon, France
L. Bottinelli
Affiliation:
Observatoire de Paris, Meudon, France
P. Chamaraux
Affiliation:
Observatoire de Paris, Meudon, France
L. Gouguenheim
Affiliation:
Observatoire de Paris, Meudon, France
J. Heidmann
Affiliation:
Observatoire de Paris, Meudon, France

Abstract

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Distance determinations of the high-redshift galaxy NGC 7319 in Stephan's Quintet, based on 21-cm line observations, yield a value much smaller than the cosmological distance. At the 98.7 % level, a part of the redshift of this galaxy which could amount to 5000 km s−1 is anomalous.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 58: The Formation and Dynamics of Galaxies , 1974 , pp. 237 - 242
Copyright
Copyright © Reidel 1974 

References

Arp, H. A.: 1973, Astrophys. J. 183, 411.Google Scholar
Balkowski, C.: 1973, Astron. Astrophys. 29, 43.Google Scholar
Balkowski, C., Bottinelli, L., Chamaraux, P., Gouguenheim, L., and Heidmann, J.: 1973, Astron. Astrophys. 25, 319.Google Scholar
Heidmann, J.: 1973, in Cayrel de Strobel, G. and Delplace, A. M. (eds.), ‘L‘âge des Etoiles’, IAU Colloq. 17, XXXVII-1.Google Scholar
Heidmann, J., Heidmann, N., and de Vaucouleurs, G.: 1972, Mem. Roy. Astron. Soc. 75, 85, 105 and 121.Google Scholar