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Mass Segregation and the Initial Mass Function of Super Star Cluster M82‐F

  • Authors: Nate McCrady, James R. Graham, and William D. Vacca

McCrady, Graham, & Vacca 2005 The Astrophysical Journal 621 278.

  • Provider: AAS Journals

Caption: Fig. 3.

Comparison of data and residuals from the fitted two‐dimensional King function. (a) ACS F814W image of M82‐F, logarithmically scaled to accentuate faint features. (b) Data image minus the fitted King function, with the same scaling as (a). Contours show the fit to the cluster at 1%, 2%, 4%, 8%, 16%, 32%, and 64% of the peak value. Scale bars in the two images represent 5 pc (0﹩\farcs﹩29) at the adopted distance of M82.

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