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Super-light motion in radio sources and its implications for the distance scale problem

Published online by Cambridge University Press:  12 April 2016

K. I. Kellermann  and
D. B. Shaffer
K. I. Kellermann
Affiliation:
National Radio Astronomy Observatory
D. B. Shaffer
Affiliation:
National Radio Astronomy Observatory

Extract

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Plusieurs radio sources comme 3C 345 et 3C 120 sont constituées de plusieurs composantes qui semblent se séparer avec une vitesse apparente de 5 ou 10 fois la vitesse de la lumière. Ce phénomène peut être interprété comme une preuve contre l’interprétation cosmologique du décalage vers le rouge. D’autres explications tirées de la physique et de la cosmologie conventionnelles sont abordées mais elles ne sont pas tout à fait satisfaisantes.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 37: Décalages vers le rouge et Expansion de l’Univers , 1977 , pp. 347 - 363
Copyright
Copyright © Editions du CNRS 1977

References

Arp, H. 1975, Pub. A.S.P., 87, 545.Google Scholar
Cohen, M. H. et al. 1971, Ap. J., 170, 207.Google Scholar
Cohen, M. H. et al. 1976, Ap. J. (Letters), 206, L1.Google Scholar
Dent, W. A. 1971, private communcation.Google Scholar
Dent, W. A. 1972, Science, 175, 1105.Google Scholar
Dent, W. A. and Kojoian, G. 1972, A. J., 77, 819.CrossRefGoogle Scholar
Dent, W. A. et al. 1974, A. J., 79, 1232.Google Scholar
Epstein, R.I. and Geller, M. J. 1976, Nature, in press.Google Scholar
Gubbay, J. et al. 1969, Nature, 224, 1094.Google Scholar
Hunstead, R. W. 1972, Ap. Letters, 12, 193.Google Scholar
Jones, T. W. and Burbidge, G. R. 1973, Ap. J., 186, 791.Google Scholar
Kellermann, K. I. and Pauliny-Toth, I. I. K. 1968, Ann. Rev. Astr. and Ap., 6, 417.CrossRefGoogle Scholar
Kellermann, K. I. and Pauliny-Toth, I. I. K. 1969, Ap. J. (Letters), 155, L71.Google Scholar
Kellermann, K. I. et al. 1973, Ap. J. (Letters), 183, L51.Google Scholar
Kellermann, K. I. et al. 1974, Ap. J. (Letters), 189, L19.Google Scholar
Kellermann, K. I. et al. 1977, Ap. J., in press.Google Scholar
Knight, C. A. et al. 1971, Science, 172, 52.Google Scholar
Legg, T. et al. 1976, Ap. J., in press.Google Scholar
Moffet, A. et al. 1972, in IAU Symposium No. 44, ed. Evans, D. S., p. 228.Google Scholar
Ozernoi, L. M. and Sazonov, V. N. 1969, Ap. and Space Sci., 3, 395.Google Scholar
Pauliny-Toth, I. I. K. and Kellermann, K. I. 1966, Ap.J., 146, 634.Google Scholar
Pauliny-Toth, I. I. K. et al. 1976, Nature, 259, 17.CrossRefGoogle Scholar
Pauliny-Toth, I. I. K. et al. 1977, in preparation.Google Scholar
Rees, M. J. 1967, M.N.R.A.S., 135, 345.Google Scholar
Schilizzi, R. T. et al. 1975, Ap. J., 201, 263.CrossRefGoogle Scholar
Seielstad, G. A. 1974, Ap. J., 193, 55.Google Scholar
Shaffer, D. B. 1973, Ph.D. Thesis.Google Scholar
Shaffer, D. B. et al. 1972, Ap. J. (Letters), 173, L147.Google Scholar
Shaffer, D. B. et al. 1975, Ap. J., 201, 256.Google Scholar
Shaffer, D. B. et al. 1977, in preparation.Google Scholar
Shapiro, I. I. et al. 1973, Ap. J. (Letters), 193, L47.Google Scholar
Whitney, A. R. et al. 1971, Science, 173, 225.CrossRefGoogle Scholar
Wittels, J. J. et al. 1976, Ap. J. (Letters), 206, L75.CrossRefGoogle Scholar