4.6 M and L of AGN Flashcards

1
Q

What is the shortest variability of an AGN?

A

1 hour from observational evidence

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2
Q

What is the typical size of an AGN, and how is calculated?

A

A few au

R_AGN < v t where v is c at most, and t is 1 hour

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3
Q

What is the concept that sets the upper limit for AGN size

A

Causality as there must be a casual connection between AGN regions due to variability

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4
Q

Define the Eddington Luminosity

A

The maximum luminosity that an object bound by gravity can have to be stable against radiation pressure

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5
Q

How is the Eddington limit calculated?

A

Balance radiation force to gravitational force

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6
Q

What is the equation for radiation force?

A

Momentum flux = flux / c multiplied by the Thomson cross section = 6.65E-29 m^2

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7
Q

What does the Eddington Luminosity allow us to deduce about AGNs?

A

They are SMBH powered by accretion

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8
Q

What is accretion?

A

Infalling of material onto an object

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9
Q

What are accretion disks?

A

The forming of material disks due to initial angular momentum

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10
Q

What causes collisions and shocks within an accretion disk?

A

The gas converting its potential energy into kinetic energy

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11
Q

What is the Schwarzchild radius?

A

The radius of a black hole

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12
Q

How efficient are black holes at converting energy?

A

50% of the rest mass can be converted into KE and radiated away
U = 1/2mc^2 when substituting the Swarzchild radius into the R in PE

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