File:Sternhaufen Anfangsbedingungen Dichteverteilung.png
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Deutsch: Anfängliche Dichteverteilung 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 Dichte ist auf diejenige im Zentrum, die Entfernung auf einen von der Größe des Haufens abhängigen Skalenfaktor R normiert. Bei einen Abstand beträgt demnach die Anfangsdichte etwa 18%, bei einen solchen circa 2% des zentralen Wertes. |
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| Source | Own work |
| Author | Michael Oestreicher |
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
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| current | 13:16, 11 August 2019 | | 1,889 × 1,417 (80 KB) | Michael Oestreicher (talk | contribs) | Corrected description of left axis |
| 17:30, 27 July 2015 |  | 597 × 407 (8 KB) | Michael Oestreicher (talk | contribs) | User created page with UploadWizard |
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