Fig. 1 from The Different Structures of the Two Classes of Starless Cores

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The Different Structures of the Two Classes of Starless Cores

Authors: Eric Keto and Paola Caselli

Keto & Caselli 2008 The Astrophysical Journal 683 238.

Provider: AAS Journals

Caption: Fig. 1.

Variation in the abundances of C, CO, and C⁺ in the photodissociation region at the edge of a cloud as calculated by the simple model described in the text. In this figure, the cloud has a constant density of 1000 cm⁻³ and the interstellar radiation field has a Habing flux, ﹩G_{0}=1﹩.

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