Symbols and units.
|βapp||c||Apparent superluminal motion|
|βint||c||Component source frame velocity|
|θ0||Degrees (°)||Viewing angle to source|
|θcrit||Degrees (°)||Critical angle, estimated from the highest observed βapp|
|BSSA||Gauss (G)||Magnetic field from SSA|
|Bequi||Gauss (G)||Minimum magnetic field from equipartition|
|T B||Kelvin (K)||Brightness temperature|
|D L||Gigaparsec (Gpc)||Luminosity distance|
|ν m||Gigahertz (GHz)||Turnover frequency|
|S m||Jansky (Jy)||Flux density at νm|
|θ m||Milliarcsecond (mas)||Angular size of emitting region at νm|
|R m||Centimeters (cm)||Linear Size of emitting region at νm|
|U rel||erg||Energy due to relativistic particles|
|U mag||erg||Energy due to magnetic fields|
|k||−||Scaling value for heavy particles|
|r||Milliarcsecond (mas)||Separation from jet base|
|R||Milliarcsecond (mas)||Transverse width of jet|
|r apex||Milliarcsecond (mas)||Separation of core from jet base|
|ΔrS||Milliarcsecond (mas)||Separation of component S from core|
Notes. A list of symbols, units and a brief description used for calculations in the paper.
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