The proper motion VS redshift relation for superluminal radio sources

Author:

Rust Bert W.,Nash Stephen G.,Geldzahler Barry J.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference27 articles.

1. B��th, L. B.: 1984, ?VLBI and Compact Radio Sources?, in R. Fanti, K. Kellerman, and G. Setti (eds.),IAU Symp. 110, 127.

2. Bahcall, J. N. and Milgrom, M.: 1980,Astrophys. J. 236, 24.

3. Bard, Yonathan: 1974,Nonlinear Parameter Estimation, Academic Press, New York.

4. Boisvert, R. F., Howe, S. E., and Kahaner, D. K.: 1984,The Guide to Available Mathematical Software (GAMS), PB 84-171305, National Technical Information Service, Springfield, VA.

5. Brent, R. P.: 1971,The Computer J. 14(4), 422.

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1. High Redshift Quasars;Annals of the New York Academy of Sciences;1995-09

2. Superluminal motion statistics and cosmology;The Astrophysical Journal;1994-08

3. Radio galaxies and quasars in cosmology;Physica Scripta;1992-01-01

4. Cosmology (Cosmologie);Transactions of the International Astronomical Union;1991

5. VLBI imaging of CTA 102;The Astrophysical Journal;1989-11

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