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Revealing Black Holes with Gaia

  • Authors: Katelyn Breivik, Sourav Chatterjee, and Shane L. Larson

2017 The Astrophysical Journal Letters 850 L13.

  • Provider: AAS Journals

Caption: Figure 4.

Distributions for the number of observable properties of BH-LCs in the MW (thin and thick disks) potentially detectable by Gaia. Histograms represent the mode of each bin height for our 500 population realizations, with shaded regions showing ﹩3\sigma ﹩ confidence limits above and below the mode. Blue, red, and black shading denote Zero-kick, FB-kick, and NS-kick models, respectively.

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