Sunday, 9 June 2013

Terminology 

beamed, beaming 
shorter terms for ‘relativistic beaming’
beta 
the ratio of the jet speed to the speed of light, sometimes called ‘relativistic beta’
core 
region of a galaxy around the central black hole
counter-jet 
the jet on the far side of a source oriented close to the line of sight, can be very faint and difficult to observe
Doppler factor 
a mathematical expression which measures the strength (or weakness) of relativistic effects in AGN, including beaming, based on the jet speed and its angle to the line of sight with Earth
flat spectrum 
a term for a non-thermal spectrum that emits a great deal of energy at the higher frequencies when compared to the lower frequencies
intrinsic luminosity 
the luminosity from the jet in the rest frame of the jet
jet (often termed 'relativistic jet')
a high velocity (close to c) stream of plasma emanating from the polar direction of an AGN
observed luminosity 
the luminosity from the jet in the rest frame of Earth
spectral index 
of measure of how a non-thermal spectrum changes with frequency, the smaller α is the more significant is the energy at higher frequencies, typically α is in the range of 0 to 2
steep spectrum 
a term for a non-thermal spectrum that emits little energy at the higher frequencies when compared to the lower frequencies

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