Evolution of a Pulsar Wind Nebula within a Composite Supernova Remnant

The interaction between a pulsar wind nebula (PWN) and its host supernova remnant (SNR) can produce a vast array of observable structures. Asymmetry present within these structures derives from the complexity of the composite system, where many factors take turns playing a dominating hand throughout...

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Veröffentlicht in:	arXiv.org 2017-07
Hauptverfasser:	Kolb, Christopher, Blondin, John, Slane, Patrick, Temim, Tea
Format:	Artikel
Sprache:	eng
Schlagworte:	Asymmetry Complexity Ejecta Gamma rays Interstellar matter Luminosity Mathematical models Morphology Nebulae Physics - High Energy Astrophysical Phenomena Pulsars Radio observation Stellar evolution Stellar winds Supernova remnants
Online-Zugang:	Volltext
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