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Hot Populations in M87 Globular Clusters

  • Authors: Sangmo T. Sohn, Robert W. O'Connell, Arunav Kundu, Wayne B. Landsman, David Burstein, Ralph C. Bohlin, Jay A. Frogel, and James A. Rose

Sohn et al. 2006 The Astronomical Journal 131 866.

  • Provider: AAS Journals

Caption: Fig. 12.

Observed ﹩( \mathrm{FUV}\,-V) _{0}﹩ colors vs. the [Fe/H] estimated from optical colors for M87 clusters (circles). Milky Way GCs are shown by triangles. The theoretical isochrones are from Fig. 6 of LLG02. With current cosmological parameters, the baseline (﹩\Delta t=0﹩) is ~12 Gyr.

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