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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. 16.

(a) Finding chart for the UV‐only sources in the near‐UV frame of field 4 for GO‐8140. A median‐filtered image has been subtracted to suppress the diffuse background. Sources that are detected in only a single epoch are enclosed by squares, while other sources are enclosed by circles; ﹩\mathrm{MJD}\,=51,315.5633﹩. (b) Same as (a), but for GO‐8780, ﹩\mathrm{MJD}\,=52,120.9713﹩. (c) Same as (a), but for GO‐8048, ﹩\mathrm{MJD}\,=52,332.2047﹩. (d) Same as (a), but for GO‐9461, ﹩\mathrm{MJD}\,=52,472.3710﹩.

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