Astrophysical Jets from accreting Black Holes

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III.1 Synchrotron Emission ● With acc= sync ⇒ max⇒ f max =3⋅10 14 2 U 3b Hz 2 c
III.2 Inverse Compton Scattering ● particles interact with the photonic background ● similar as for the sychrotron emission it follows considering both effects: f max =3⋅10 14 3b U2 f a Hz 2 c where a is the ratio of photonic to magnetic energy density
Page 1 and 2: Astrophysical Jets from accreting B
Page 3 and 4: I.Description of astrophysical jets
Page 5 and 6: I.1 Sources of Jets Active Galaxy N
Page 7 and 8: I.1 Sources of Jets Gamma Ray Burst
Page 9 and 10: I.3 Formation Mechanism ● not kno
Page 11 and 12: II. Acceleration in Jets
Page 13 and 14: II.2 Diffusive shock acceleration
Page 35: III.1 Synchrotron Emission ● part
Page 39 and 40: III.3 Other Processes ● 1. proton
Page 41: II.2 Diffusive shock acceleration

Astrophysical Jets from accreting Black Holes

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