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Cloud Structure and Physical Conditions in Star‐forming Regions from Optical Observations. II. Analysis

  • Authors: K. Pan, S. R. Federman, Y. Sheffer, and B-G Andersson

Pan et al. 2005 The Astrophysical Journal 633 986.

  • Provider: AAS Journals

Caption: Fig. 9.

Logarithmic plots of total column densities along lines of sight in Cep OB2 and Cep OB3. The error bars represent 10% uncertainties in N. Top: N(CH) vs. N(H2). The solid line shows the best fit to Cep OB2 data. Bottom: N(CO) vs. N(H2). The solid line represents the best fit to Cep OB2 data, and the dashed line to Cep OB3 data. Note that, for a given N(H2), Cep OB2 sight lines have higher CH and CO column densities than lines of sight toward Cep OB3.

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