Fig. 5 from Mid‐Infrared Emission Features in WL 16

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Mid‐Infrared Emission Features in WL 16

Authors: B. DeVito and T. L. Hayward

DeVito & Hayward 1998 The Astrophysical Journal Letters 504 L43.

Provider: AAS Journals

Caption: Fig. 5.

Comparison of WL 16 to other astrophysical sources in terms of the [8.6]/[11.3] ratio vs. the integrated 6–13 eV flux field intensity, given in terms of the Habing field: ﹩G_{0}=1.6\times 10^{-3}﹩ ergs cm⁻² s⁻¹ (Habing 1968).

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