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This thesis is the first extensive photometric and spectroscopic survey of star clusters in the nearby late-spiral galaxy M33, a key example of dwarf spiral galaxies. It aims to understand M33's formation and evolution, presenting a comprehensive catalog of star clusters and concluding that M31 has likely influenced M33's evolution.
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The Formation and Evolution of M33 as Revealed by Its Star Clusters, Izaskun San Roman
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- Publicado en
- 2015
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