Fig. 2 from Far Ultraviolet Spectroscopic Explorer Observations of Diffuse Interstellar Molecular Hydrogen

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Far Ultraviolet Spectroscopic Explorer Observations of Diffuse Interstellar Molecular Hydrogen

Authors: J. Michael Shull, Jason Tumlinson, Edward B. Jenkins, H. Warren Moos, Brian L. Rachford, Blair D. Savage, Kenneth R. Sembach, Theodore P. Snow, George Sonneborn, Donald G. York, William P. Blair, James C. Green, Scott D. Friedman, and David J. Sahnow

Shull et al. 2000 The Astrophysical Journal Letters 538 L73.

Provider: AAS Journals

Caption: Fig. 2.

Left: Composite curve of growth for 28 H₂ lines (﹩J=0,\,1,\,2,\,3﹩) in the SMC (+120 km s⁻¹) component toward HD 5980 with best‐fit Doppler parameter ﹩b=10﹩ km s⁻¹ and column densities N(J). Right: Same 28 FUSE lines, but with the higher ORFEUS column densities for ﹩J=0﹩, 1, 2 (see Richter et al. 1998, who used ﹩b=6﹩ km s⁻¹).

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