Image Details

Choose export citation format:

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 8.

(a) Number distribution of source counts for the GCs: crosses: X-ray-undetected GCs; diamond: X-ray-detected GCs with fluxes below the detection completeness limit. The histogram is a representation of the number distribution of local background counts. The curve shows the predicted number distribution from the best-fit model NFR. See the text for details. (b) The 68%, 90%, and 99% confidence contours of the faint-end index and the break flux. The plus sign marks the best-fit values. The vertical dashed line marks the best-fit value of the bright-end index derived from the X-ray-detected GCs.

Other Images in This Article
Copyright and Terms & Conditions