Unified Models: 
Different Views of the Accretion Disk
–The torus of gas and dust can block part of our view
•Seyfert 2 galaxies: Edge on view
Only gas well above and below disk is visible
See only “slow” gas Þ narrow emission lines
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•Seyfert 1 galaxies: Slightly tilted view
Hot high velocity gas close to black hole is visible
High velocities   Þ broad emission lines
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•BL Lac objects: Pole on view
Looking right down the jet at central region
Extremely bright – vary on time scales of hours
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•Quasars: Very active AGN at large distances
Can barely make out the galaxy surrounding them
Were apparently more common in distant past
From our text:  Horizons, by Seeds