burgeon
发表于 2025-3-21 17:08:06
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Asparagus
发表于 2025-3-21 21:33:42
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Inoperable
发表于 2025-3-22 04:08:27
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为宠爱
发表于 2025-3-22 05:46:04
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Gesture
发表于 2025-3-22 11:05:53
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有效
发表于 2025-3-22 15:40:44
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Ossification
发表于 2025-3-22 19:10:23
Riccardo Bassoli,Holger Boche,Christian Deppe,Roberto Ferrara,Frank H. P. Fitzek,Gisbert Janssen,Sajf such simulations represent a good match to the observations. This issue is not entirely straightforward given the complex morphology and hierarchical nature of observed molecular clouds (and also of numerical simulations). For example, the fact that simulations generally produce filamentary and hi
Hla461
发表于 2025-3-22 22:02:41
Riccardo Bassoli,Holger Boche,Christian Deppe,Roberto Ferrara,Frank H. P. Fitzek,Gisbert Janssen,Sajch simulations are informed by observations of the gas in Giant Molecular Clouds (GMCs). We therefore present a brief overview of the properties of GMCs and how these are deduced observationally, focussing in particular on the three inter-related ‘Larson’ relations. We emphasise the dynamical import
连系
发表于 2025-3-23 05:14:04
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机制
发表于 2025-3-23 08:43:29
(such as an open or globular cluster), or disperses to join the field stars in the disc of the Galaxy? These questions not only impact understanding of the origins of stars and planetary systems like our own (and the potential for life to emerge that they represent), but also galaxy formation and ev