Figure 1 from EXPLORING THE OVERABUNDANCE OF ULXs IN METAL- AND DUST-POOR LOCAL LYMAN BREAK ANALOGS

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EXPLORING THE OVERABUNDANCE OF ULXs IN METAL- AND DUST-POOR LOCAL LYMAN BREAK ANALOGS

Authors: Antara R. Basu-Zych, Bret Lehmer, Tassos Fragos, Ann Hornschemeier, Mihoko Yukita, Andreas Zezas, and Andy Ptak

2016 The Astrophysical Journal 818 140.

Provider: AAS Journals

Caption: Figure 1.

HST image of our two LBAs: VV 114 (left), Haro 11 (right). Magenta circles mark the 2–10 keV source detections, with the circle size scaling with the X-ray luminosity. The red crosses on VV 114 and Haro 11 mark sources that we consider potential accreting SMBHs (see Section 3.4).

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