Low-frequency variability and predicted superluminal motion in 3C147

Details Low-frequency variability and predicted superluminal motion in 3C147 Low-frequency variability and predicted superluminal motion in 3C147

Apr 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983natur.302..487s&link_type=abstract

Nature (ISSN 0028-0836), vol. 302, April 7, 1983, p. 487-490.

Computer Science

Performance

23

Extragalactic Radio Sources, Radio Sources (Astronomy), X Ray Sources, Brightness Temperature, Low Frequencies, Performance Prediction, Radiation Transport, Relativistic Particles, Variability, Very Long Base Interferometry, X Ray Astronomy

Scientific paper

VLBI observations of 3C 147 reveal that its core is a low-frequency variable radio source which has brightened by a factor of 2 in 6 years. In combination with X-ray observations, this implies that bulk relativistic motion is taking place within the core, and leads to the prediction that 3C 147 is a member of the class of superluminal radio sources.

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