Results 161 to 170 of about 2,467 (183)
Synchrotron intensity gradient revealing magnetic fields in galaxy clusters. [PDF]
Hu Y +5 more
europepmc +1 more source
A Metric for the Entropic Purpose of a System. [PDF]
Parker MC, Jeynes C, Walker SD.
europepmc +1 more source
Some of the next articles are maybe not open access.
Related searches:
Related searches:
Resonance, 2018
Jets in active galaxies are signatures of energy supply via collimated beams of plasma from the galactic nucleus to the extended regions of emission. These jets, which occur across the electromagnetic spectrum, are powered by supermassive black holes in the centres of the host galaxies.
openaire +1 more source
Jets in active galaxies are signatures of energy supply via collimated beams of plasma from the galactic nucleus to the extended regions of emission. These jets, which occur across the electromagnetic spectrum, are powered by supermassive black holes in the centres of the host galaxies.
openaire +1 more source
Are There Jets in Spiral Galaxies?
1983The absence in spiral galaxies of large-scale collimated jets of radio emission is still little understood. Collimated emission in elliptical galaxies in some cases exceeds by far the optical extent of the galaxy (e.g. in NGC6251). Westerbork observations of NGC4258 (van der Kruit, Oort and Mathewson, 1972) and NGC3079 (de Bruyn, 1977) have provided ...
C. Kotanyi, E. Hummel, J. van Gorkom
openaire +1 more source
Classification of Optical Jets in Galaxies
1986New, deep images of galaxies reported in various catalogs to have optical jets show that most are not jets, but tidal features, polar rings, or superpositions. From those objects that do seem to represent nuclear ejecta, criteria of brightness relative to the parent galaxy, width, and location have been derived, which should produce much purer samples ...
openaire +1 more source
The Jets in Radio Galaxy B1308–441
Publications of the Astronomical Society of Australia, 1996AbstractThe giant radio galaxy B1308–441 has prominent two-sided jets, typical of Fanaroff–Riley class I radio galaxies, but there is an unusual bright spot in the SE jet 2 arcmin from the core that gives a marked asymmetry to the source. Observations at 1·37 and 2·37 GHz with the Australia Telescope Compact Array show that the bright spot has a ...
openaire +1 more source
Heat transfer intensification of jet impingement using exciting jets - A comprehensive review
Renewable and Sustainable Energy Reviews, 2021Hussein M Maghrabie
exaly

