Poster Open Access
Using statistical methods to investigate the kinematic and spatial history of star clusters.
Arnold, Becky;
Wright, Nick
Editor(s)
Wolk, ScottThe dynamical history of young star forming regions is a difficult thing to study because kinematic structure is quickly erased as the regions evolve. We explore the application of the Moran's I statistic to look for kinematic signatures of this initial structure which persist. The ability to diagnose a cluster's evolutionary origins and history would be a powerful tool in distinguishing which models of star formation best reflect reality.
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Becky_Arnold_poster.pdf
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Portegies Zwart et al. (1999) Star cluster ecology. III. Runaway collisions in young compact star clusters
Portegies Zwart et al. (2001) Star cluster ecology - IV. Dissection of an open star cluster: photometry
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| Views | 64 | 64 |
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| Data volume | 98.1 MB | 98.1 MB |
| Unique views | 60 | 60 |
| Unique downloads | 66 | 66 |
- Publication date:
- February 25, 2021
- DOI:
-
- Keyword(s):
- Stellar systems, clusters, and associations Stellar dynamics Statistical methods
- Meeting:
- The 20.5th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun (CS20.5), March 2-4, 2021
- Communities:
- License (for files):
- Creative Commons Attribution 4.0 International