Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981mnras.196..481b&link_type=abstract
Monthly Notices of the Royal Astronomical Society, vol. 196, Aug. 1981, p. 481-489. Research supported by the Max-Planck-Instit
Astronomy and Astrophysics
Astronomy
3
Beams (Radiation), Electromagnetic Wave Transmission, Nonuniform Plasmas, Radio Sources (Astronomy), Refracted Waves, Astronomical Models, Density Distribution, Galactic Nuclei, Ray Tracing, Space Density
Scientific paper
An interpretation of bridge bending in head-tail radio sources in the framework of an electromagnetic beam model is presented. The physical effect responsible for the structural distortion is proposed to be the refraction of a large-amplitude wave in a medium with a density gradient perpendicular to the wave propagation vector; this gradient is consistently produced by the relative motion of the beam source in the surrounding medium with a velocity higher than the speed of sound. These effects are calculated in some detail and a quantitative fit of model parameters to the typical radio source associated with NGC 1265 is discussed.
Bodo Gianluigi
Ferrari Aldo
Massaglia Silvano
No associations
LandOfFree
Bending of electromagnetic beams and head-tail 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 Bending of electromagnetic beams and head-tail radio sources, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Bending of electromagnetic beams and head-tail radio sources will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1747586