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X-ray Emission from the Sombrero Galaxy: Discrete Sources

  • Authors: Zhiyuan Li, Lee R. Spitler, Christine Jones, William R. Forman, Ralph P. Kraft, Rosanne Di Stefano, Shikui Tang, Q. Daniel Wang, Marat Gilfanov, and Mikhail Revnivtsev

LI et al. 2010 The Astrophysical Journal 721 1368.

  • Provider: AAS Journals

Caption: Figure 4.

0.4–6 keV count rate vs. (a) V-band magnitude and (b) hardness ratio for the GC-LMXBs. The hardness ratio is defined as HR = ( H2 − MS1)/( H2 + M + S1). Blue and red GCs are plotted with blue triangles and red open circles, respectively. The UCD is plotted with a filled circle for comparison. The horizontal dashed line in panel (a) represents the Eddington luminosity of an accreting NS with a mass of 1.4  M . The vertical dashed lines in panel (b), from left to right, correspond to hardness ratios for an absorbed power-law spectrum with a fixed N H = 10 21 cm −2 and a photon index of 2.0, 1.7, and 1.4, respectively.

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