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28 March 2024
 
  » arxiv » astro-ph/0010168

 Article overview


WFPC2 Observations of Massive and Compact Young Star Clusters in M31
Benjamin F. Williams ; Paul W. Hodge ;
Date 9 Oct 2000
Subject astro-ph
AbstractWe present color magnitude diagrams of four blue massive and compact star clusters in M31: G38, G44, G94, and G293. The diagrams of the four clusters reveal a well-populated upper main sequence and various numbers of supergiants. The U-B and B-V colors of the upper main sequence stars are used to determine reddening estimates of the different lines of sight in the M31 disk. Reddening values range from E(B-V) = 0.20 +/- 0.10 to 0.31 +/- 0.11. We statistically remove field stars on the basis of completeness, magnitude and color. Isochrone fits to the field-subtracted, reddening-corrected diagrams yield age estimates ranging from 63 +/- 15 Myr to 160 +/- 60 Myr. Implications for the recent evolution of the disk near NGC 206 are discussed.
Source arXiv, astro-ph/0010168
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