Stationary relativistic MHD flows: Accretion to rotating black holes and formation of relativistic jets

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Bibliographische Detailangaben
1. Verfasser: Camenzind, Max (VerfasserIn)
Dokumenttyp: Kapitel/Artikel Konferenzschrift
Sprache:Englisch
Veröffentlicht: 1996
In: Solar and astrophysical magnetohydrodynamic flows
Year: 1996, Pages: 699-725
Schlagworte:
Online-Zugang: Volltext
Verfasserangaben:M. Camenzind

MARC

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