Probability approach to the ballistic models of superluminal radio sources

Details Probability approach to the ballistic models of superluminal radio sources Probability approach to the ballistic models of superluminal radio sources

May 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.133..149p&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 133, no. 1, May 1987, p. 149-155.

Mathematics

Probability

1

Light Speed, Probability Theory, Quasars, Radio Sources (Astronomy), Seyfert Galaxies, Very Long Base Interferometry, Angular Resolution, High Resolution, Spherical Coordinates, Statistical Analysis

Scientific paper

A probability approach is used to examine the plausibility of ballistic models as the explanation for the superluminal phenomenon observed in extragalactic sources including the quasars 3C 273, 3C 279, and 3C 345 and the nucleus of Seyfert galaxy 3C 120. The analysis is applied to four two-component models for the sources: (1) a stationary and an ultrarelativistic source; (2) two ultrarelativistic sources; (3) a stationary source and a tachyonic source; and (4) two tachyonic sources. The low probability found for all four models argues against the ballistic description of superluminal sources.

Affiliated with

Also associated with

No associations

Rating

Probability approach to the ballistic models of superluminal 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 Probability approach to the ballistic models of superluminal radio sources, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Probability approach to the ballistic models of superluminal radio sources will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-856681