DYNAMICAL EVOLUTION OF BINARY STAR CLUSTER FORMATION IN MILKY WAY AND LARGE MAGELLANIC CLOUD FROM FRACTAL MODEL
<p align="justify">MIStIX survey showed that most of young star clusters (a few Myr) have clumpy structures. Observations and statistical studies also concluded that there are binary star clusters in Milky Way and Large Magellanic Cloud. Their typical ages are less than 25 Myr. Some...
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| 格式: | Theses |
| 語言: | Indonesia |
| 在線閱讀: | https://digilib.itb.ac.id/gdl/view/30313 |
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