Fig. 3
Top: the distribution of dynamically confirmed BHs (circles) and BH candidates (stars) in the Galactic plane, using the Hammer projection. (Background image credit: Mellinger 2009). Some of the symbols are overlapped by others, especially in the Galactic centre region. Bottom: histogram of the distribution of BH transients in Galactic longitude (left) and latitude (right). A 10° bin size in longitude and 5° bin in latitude were used respectively.
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