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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. 1.

Four observed HST STIS fields, superposed on a WFPC2 image of the inner region of M87. To remove the diffuse background, a median‐filtered image was subtracted from the original WFPC2 image. The entire field of view of the image is ﹩160^{\prime \prime }\times 160^{\prime \prime }﹩. Locations of the nucleus and optical jet of M87 are indicated. Most of the point sources shown in the figure are GCs. The centers of fields 1, 2, 3, and 4 are located at angular distances of 38﹩\arcsec﹩, 73﹩\arcsec﹩, 22﹩\arcsec﹩, and 10﹩\arcsec﹩, respectively, from the nucleus of M87.

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