Kinematics of subclusters in star cluster complexes: imprint of their parental molecular clouds
ABSTRACT Star cluster complexes such as the Carina Nebula could have formed in turbulent giant molecular clouds. We perform a series of N-body simulations starting from subclustering initial conditions based on hydrodynamic simulations of turbulent molecular clouds. These simulations finally result...
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| Veröffentlicht in: | Monthly notices of the Royal Astronomical Society 2019-07, Vol.486 (3), p.3019-3026 |
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| Format: | Artikel |
| Sprache: | eng |
| Online-Zugang: | Volltext |
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