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Spectral Microlensing of Extragalactic H II Regions by Stellar-mass Black Holes

  • Authors: Dezi Liu

Dezi Liu 2026 The Astrophysical Journal Letters 1007 .

  • Provider: AAS Journals

Caption: Figure 3.

Top panel: physical size upper limit ﹩{R}_{S}^{{\rm{\max }}}﹩ of background H II regions as a function of source redshift zS (or DS). The solid and dashed black curves denote the mean ﹩{R}_{S}^{{\rm{\max }}}﹩ for BHs in the Galactic disk and halo, respectively. The light and dark shaded regions enclose the full range (from minimum to maximum) of ﹩{R}_{S}^{{\rm{\max }}}﹩ for each component. Bottom panel: optical depth τ contributed by disk (solid lines) and halo (dashed lines) BHs. Thick lines are for compact H II regions, while thin lines are for extended ones.

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