File:Das Mehrkörperproblem in der Astronomie Haufen initiale Geschwindigkeitsverteilung.png

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Das_Mehrkörperproblem_in_der_Astronomie_Haufen_initiale_Geschwindigkeitsverteilung.png (554 × 408 pixels, file size: 8 KB, MIME type: image/png)

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Deutsch: Anfängliche Geschwindigkeitsverteilung in Sternhaufen nach Angaben von Aarseth S.J., Henon M, Wielen R., in: A Comparison of Numerical Methods for the Study of Star Cluster Dynamics, Astronomy and Astrophyscia Band 37, S.183ff, 1974. Die Geschwindigkeit ist auf die Fluchtgeschwindigkeit normiert, welche in einem bestimmten Abstand r vom Zentrum des Haufens vorliegt. Die Fluchtgeschwindigkeit variiert selbstverständlich mit r, doch die Form der initialen Geschwindigkeitsverteilung ist dem von den Autoren benutzten Modell zufolge überall im Haufen gleich.
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