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Properties of Resolved Star Clusters in M51

  • Authors: Myung Gyoon Lee, Rupali Chandar, and Bradley C. Whitmore

Lee, Chandar, & Whitmore 2005 The Astronomical Journal 130 2128.

  • Provider: AAS Journals

Caption: Fig. 5.

Derived age vs. mass for our NGC 5194 cluster sample. The solid line shows how our detection limit of ﹩V=22﹩ affects our ability to detect star clusters as a function of age.

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