Star Formation and Relaxation in 379 Nearby Galaxy Clusters
  We investigate the relationship between star formation (SF) and level of
relaxation in a sample of 379 galaxy clusters at z < 0.2. We use data from the
Sloan Digital Sky Survey to measure cluster membership and level of relaxation,
and to select star-forming galaxies based on mid-infrared emission detected
with the Wide-Field Infrared Survey Explorer. For galaxies with absolute
magnitudes M_r < -19.5, we find an inverse correlation between SF fraction and
cluster relaxation: as a cluster becomes less relaxed, its SF fraction
increases. Furthermore, in general, the subtracted SF fraction in all unrelaxed
clusters (0.117 +/- 0.003) is higher than that in all relaxed clusters (0.097
+/- 0.005). We verify the validity of our SF calculation methods and membership
criteria through analysis of previous work. Our results agree with previous
findings that a weak correlation exists between cluster SF and dynamical state,
possibly because unrelaxed clusters are less evolved relative to relaxed
clusters.
