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Stratified Wind Geometries of GRS 1915+105: Density Profiles and Radii

  • Authors: Noa Keshet, Ehud Behar, Jon M. Miller, Joey Neilsen

Noa Keshet et al 2026 The Astrophysical Journal 1010 .

  • Provider: AAS Journals

Caption: Figure 3.

(Top panel) Distribution of measured ionic column densities Nion in the GRS 1915+105 outflow of observations 23435+24663, each plotted at its ξ of maximal formation. This outlines the overall distribution of NH with ξ, showing a gradual increase, and then a turnover. The dashed lines represent the local slopes from H-like and He-like ion pairs, which are used to reconstruct the continuous AMD (see text), plotted in the bottom panel. Since there is no H in the spectrum, fion(ξ) and AZ of H-like Fe are used to scale the absolute AMD values in terms of NH (Equation (3)).

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