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HD 62542: Probing the Bare, Dense Core of a Translucent Interstellar Cloud

  • Authors: Daniel E. Welty, Paule Sonnentrucker, Theodore P. Snow, and Donald G. York

2020 The Astrophysical Journal 897 36.

  • Provider: AAS Journals

Caption: Figure 10.

Column densities of CH, CH+, 12CO, and CN vs. N(H2), for Galactic sight lines. The large red star denotes the sight line toward HD 62542 (main component); the open diamonds denote Pleiades sight lines. The solid lines show weighted and unweighted fits to the data; the dotted lines represent the models of van Dishoeck & Black (1988, 1989); the three models for 12CO are (left to right) for IUV = 0.5, 1.0, and 10 times the average local Galactic radiation field. Relative to the mean trends with N(H2), Nm(CH) is “normal” toward HD 62542, Nm(CH+) is very low, and Nm(12CO) and Nm(CN) are high.

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