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Particle acceleration at relativistic shock waves - cont.

Lecture 4. Particle acceleration at relativistic shock waves - cont. Ultra-relativistic shock waves. superluminal (perpendicular) shocks, u B,1 > c. Considered objects: - mechanism of GRB generation - pulsar wind terminal shock - shocks in AGN sub-parsec scale jets.

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Observed radio - PowerPoint PPT Presentation

Particle acceleration at relativistic shock waves - cont.