SSC

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  • Dowell et al.
  • http://arxiv.org/abs/astro-ph/0611586
  • SSCs in nearby spirals and irregulars from SDSS
  • SDSS colors plus spectral evolutionary modelling to determine cluster ages and mass.
  • They find a steeper slope for the mass function (at high masses) in irregulars as compared to spirals.
  • I wonder how reliable the masses are from this method. It’s a tricky business and dynamical cluster masses would be nicer.

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