Fig. 2 from Cloud Structure and Physical Conditions in Star‐forming Regions from Optical Observations. II. Analysis

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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. 2.

Logarithmic plots of column densities. The error bars represent 20% uncertainties in N. Top: N(CN) vs. N(CH⁺‐corrected CH). The solid line presents the best fit with a slope of 1.73, indistinguishable from the one between N(CN) and N(CN‐like CH). Bottom: N(CN) vs. N(CN‐like CH).

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