Fig. 6 from The Galactic Halo’s O VI Resonance Line Intensity

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The Galactic Halo’s O VI Resonance Line Intensity

Authors: Robin L. Shelton, Shauna M. Sallmen, and Edward B. Jenkins

Shelton, Sallmen, & Jenkins 2007 The Astrophysical Journal 659 365.

Provider: AAS Journals

Caption: Fig. 6.

Radiative energy loss rates per unit area, ﹩dU/ dt﹩, as a function ﹩\mathrm{log}\,T﹩ for the preferred values of β that apply to the three possible values of the foreground N(H I) (see Table 4). The curves plotted represent the product of the integrand and constants given in eq. (15).

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