Magnetic Rayleigh-Taylor instability for Pulsar Wind Nebulae in expanding Supernova Remnants (Q57953311)
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scientific article published in Astronomy and Astrophysics
Language | Label | Description | Also known as |
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English | Magnetic Rayleigh-Taylor instability for Pulsar Wind Nebulae in expanding Supernova Remnants |
scientific article published in Astronomy and Astrophysics |
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Magnetic Rayleigh-Taylor instability for Pulsar Wind Nebulae in expanding Supernova Remnants (English)
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29 July 2004
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