Comments on the superluminal motion in Cygnus X-3
R. N. Ogley, S. J. Bell Burnell, S. J. Newell
Abstract
Open-access reader
R. N. Ogley, S. J. Bell Burnell, S. J. Newell
Abstract
Open-access reader
Following the recent discovery that Cyg X-3 exhibits superluminal motion, the implications of superluminal expansion and contraction are investigated. We propose that the effect is due to either a propagating photon pattern or to outwardly moving shells illuminated by an intense beam of radiation.
OpenAlex reports 3 citations for this work. Citation counts describe recorded attention and do not establish research quality.
A contribution statement is not available in the OpenAlex record.
Method details are not available in the OpenAlex metadata.
Findings are not separately available in the OpenAlex metadata.
Limitations are not available in the OpenAlex metadata.
Application details are not available in the OpenAlex metadata.
Following the recent discovery that Cyg X-3 exhibits superluminal motion, the implications of superluminal expansion and contraction are investigated. We propose that the effect is due to either a propagating photon pattern or to outwardly moving shells illuminated by an intense beam of radiation.
Key concepts: Superluminal motion, Physics, Astrophysics, Motion (physics), Astronomy, Proper motion, Radiation, Classical mechanics