On the structure of stellar clusters after relaxation
The evolution of globular clusters is studied by means of N -body problem calculations with 16 and 25 stars for time intervals up to 40 times of relaxation. It is found that within two to four times of relaxation all clusters with different starting conditions approach an isothermal polytrope and a...
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| Veröffentlicht in: | Symposium - International Astronomical Union 1966, Vol.25, p.146-154 |
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| Format: | Artikel |
| Sprache: | eng |
| Online-Zugang: | Volltext |
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