Modeling the Galactic Center Nonthermal Filaments as Magnetized Wake

We simulate the Galactic Center nonthermal filaments as magnetized wakes formed dynamically from amplification of a weak (tens of \(\mu\)G) global magnetic field through the interaction of molecular clouds with a Galactic Center wind. One of the key issues in this cometary model is the stability of...

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Veröffentlicht in:	arXiv.org 2001-12
Hauptverfasser:	Dahlburg, Russell B, Einaudi, Giorgio, LaRosa, T N, Shore, Steven N
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomical models Comets Computer simulation Dimensional stability Disruption Dynamic stability Filaments Interstellar Molecular clouds Shredding Star & galaxy formation Wakes
Online-Zugang:	Volltext
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