Fanaroff–Riley classification

The Fanaroff–Riley classification is a scheme created by
Fanaroff-Riley Class I (FR-I)
These sources are brighter towards their central galaxy or quasar and become fainter toward the outer extremities of the lobes (also called edge-darkened). The spectra here are steepest, indicating that the radiating particles have aged the most. Jets are detected in a large majority of FR-I galaxies, and these hosts also tend to be bright, large galaxies often located in rich clusters with extreme X-ray emitting gas. As the galaxy moves through the cluster, the gas can sweep back and distort the radio structure through ram pressure.
Fanaroff-Riley Class II (FR-II)
This class of sources are also known as edge-brightened and are more luminous than their counterparts, with bright hotspots at the ends of their lobes. The jets are often one-sided due to relativistic beaming.
See also
References
- doi:10.1093/mnras/167.1.31p.)
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: CS1 maint: multiple names: authors list (link - ISBN 9783642005763. Retrieved 2013-01-11.
- ^ "Fanaroff-Riley Classification". NASA/IPAC Extragalactic Database (NED). Caltech. Retrieved 11 January 2013.