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Probing the GC LMXB Connection in NGC 1399: A Wide field Study with the Hubble Space Telescope and Chandra

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Figure

Figure 1. Illustration of the 3 × 3 mosaic of our ACS observations (black solid lines) overplotted on a DSS-2 image of the NGC 1399 region
Figure 2. Luminosity distributions of optical and X-ray point-like sources (e.g., with stellarity index <0.9) within the HST FOV
Figure 6). The properties of the closest optical counterpart for each X-ray source are reported in Table 4.
Figure 4. Fraction of GCs hosting LMXBs as a function of luminosity. The two panels show parametrizations of those fractions by galactocentric distance (upper panel) or GC color (lower panel)
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