Non-thermal emission from relativistic MHD simulations of pulsar wind nebulae: from synchrotron to inverse Compton (Q3519250)
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| Language | Label | Description | Also known as |
|---|---|---|---|
| English | Non-thermal emission from relativistic MHD simulations of pulsar wind nebulae: from synchrotron to inverse Compton |
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Non-thermal emission from relativistic MHD simulations of pulsar wind nebulae: from synchrotron to inverse Compton (English)
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14 August 2008
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radiation mechanisms: non-thermal
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magnetohydrodynamics (MHD)
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relativity
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stars: pulsars: general
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ISM: supernova remnants
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ISM: individual objects: Crab Nebula
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