|  | 
   
    |  |  |  |  |  |  |  |  |  |  |  |  |  |  |  |  |  |  
    | • | Compact
    Sources (arcsecond scales and smaller) 
 |  |  
    |  |  
    | • | Extended
    Sources (Fanaroff-Riley 1974 classes) and 
 |  |  
    |  | can
    be very large (many arcminutes, up to Mpc) 
 |  |  
    |  |  
    |  | – | FR I,
    tend to be lower power, continuous, jets 
 |  |  
    |  | • | BL
    Lacs, radio galaxies 
 |  |  
    |  |  
    |  | – | FR
    II, higher power, edge-brightened lobes 
 |  |  
    |  | • | Quasars,
    radio galaxies 
 |  |  
    |  | – | Other
    stuff.  More messes, oh yes!  Messes in deep space. 
 |  |  
    |  |  
    | • | Optical
    IDs 
 |  |  
    |  | – | Tough
    game historically – point sources, (elliptical) galaxies 
 |  |  |