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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 5.

HR1 vs. HR2, where HR1 = ( H1 − S2 − S1)/( H1 + S2 + S1) and HR2 = ( H2 − H1)/( H2 + H1). The blue and red symbols are the same representation of GC-LMXBs as in Figure 4(a), whereas black crosses represent those field X-ray sources detected within R = 4′ and simultaneously detected in the F, M, and H2 bands. For clarity, error bars are not shown for the field sources, which have a similar uncertainty range as those of the GC-LMXBs.

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