Star Clusters Driven to Form by Strong Collisions Between Gas Clouds in High-Velocity Random Motion
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Cited by 36 articles. 订阅此论文施引文献 订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献
1. A clustering (DBSCAN+GMM) investigation of the young open cluster NGC 6649;Monthly Notices of the Royal Astronomical Society;2023-11-02
2. Pearls on a String: Numerous Stellar Clusters Strung Along the Same Orbit;The Astrophysical Journal;2022-03-01
3. Disruption of Hierarchical Clustering in the Vela OB2 Complex and the Cluster Pair Collinder 135 and UBC 7 with Gaia EDR3: Evidence of Supernova Quenching;The Astrophysical Journal;2021-12-01
4. Collinder 135 and UBC 7: A physical pair of open clusters;Astronomy & Astrophysics;2020-10
5. Ultra-diffuse galaxies without dark matter;Monthly Notices of the Royal Astronomical Society: Letters;2019-07-01
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