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Ultraviolet Properties of Galactic Globular Clusters with GALEX. I. The Color-Magnitude Diagrams

  • Authors: Ricardo P. Schiavon, Emanuele Dalessandro, Sangmo T. Sohn, Robert T. Rood, Robert W. O'Connell, Francesco R. Ferraro, Barbara Lanzoni, Giacomo Beccari, Soo-Chang Rey, Jaehyon Rhee, R. Michael Rich, Suk-Jin Yoon, and Young-Wook Lee

Schiavon et al. 2012 The Astronomical Journal 143 121.

  • Provider: AAS Journals

Caption: Figure 14.

Stacked color–magnitude diagram of 23 Galactic GCs (see Section 4). The UV-bright population composed by candidate post-He-core burning at ( M FUVM NUV) ~ 0 and  M FUV ≲ 2  is clearly seen in this stack. Redder stars brighter than the HB are likely to be predominantly background sources. The blue stragglers can also be very clearly spotted in this diagram, below the redder half of the HB.

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