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Optical Studies of the Ultraluminous X‐Ray Source NGC 1313 X‐2

  • Authors: Ji-Feng Liu, Joel Bregman, Jon Miller, and Philip Kaaret

Liu et al. 2007 The Astrophysical Journal 661 165.

  • Provider: AAS Journals

Caption: Fig. 4.

Color‐magnitude diagrams for the ULX counterpart and nearby bright stars. Both the data and isochrones are in the HST ACS/WFC VEGAmag system. The magnitudes are corrected for the Galactic extinction of ﹩E( B-V) =0.11﹩ mag. (a) MF555W vs. ﹩\mathrm{F}\,435\mathrm{W}\,-\mathrm{F}\,555\mathrm{W}\,﹩. The ages for the isochrones are 107, ﹩5\times 10^{7}﹩, ﹩2\times 10^{8}﹩, and ﹩5\times 10^{8}﹩ yr, respectively. (b) MF555W vs. ﹩\mathrm{F}\,555\mathrm{W}\,-\mathrm{F}\,814\mathrm{W}\,﹩. The ages for the isochrones are 107, ﹩5\times 10^{7}﹩, ﹩3\times 10^{8}﹩, 109, and ﹩3\times 10^{9}﹩ yr, respectively.

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