Superluminal motion in compact radio sources

Details Superluminal motion in compact radio sources Superluminal motion in compact radio sources

Apr 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980pasp...92..127m&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 92, Apr.-May 1980, p. 127-133. NASA-NSF-supported research.

Astronomy and Astrophysics

Astrophysics

31

Astronomical Models, Quasars, Radio Sources (Astronomy), Stellar Motions, Astrophysics, Detonation Waves, Galaxies, Plasma Jets, Relativistic Effects

Scientific paper

The observations of radio sources whose components appear to move superluminally are now sufficient to eliminate certain theoretical models. However, a number of models might be still relevant. The models which involve relativistic bulk motions of the radio components seem to provide the most likely explanation of apparent superluminal motion. A summary of observational predictions of various models for superluminal motions is included.

Affiliated with

Also associated with

No associations

Rating

Superluminal motion in compact radio sources does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Superluminal motion in compact radio sources, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Superluminal motion in compact radio sources will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1699529