Figure 3 from New Tests for Disruption Mechanisms of Star Clusters: Methods and Application to the Antennae Galaxies

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New Tests for Disruption Mechanisms of Star Clusters: Methods and Application to the Antennae Galaxies

Authors: S. Michael Fall, Rupali Chandar, and Bradley C. Whitmore

FALL, CHANDAR, & WHITMORE 2009 The Astrophysical Journal 704 453.

Provider: AAS Journals

Caption: Figure 3.

Mass function of Antennae clusters in the indicated intervals of age. The lines are power laws, dN/ dM ∝ M ^β, with best-fit exponents β = −2.14 ± 0.03 (dashed) and β = −2.03 ± 0.07 (solid) for the younger and older clusters, respectively.

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