Image Details

Choose export citation format:

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. 1.

Logarithmic plots of column densities. The error bars represent 20% uncertainties in N. Top: N(CN) vs. N(CH). The solid line presents our best fit. Bottom: N(CH+‐like CH) vs. N(CH+). The solid line is the best fit to components with ﹩\mathrm{log}\,N( \mathrm{CH}\,^{+}) \leq 12.6﹩ (see text for more detail). Here, and elsewhere, components toward Cep OB2 (asterisks), Cep OB3 (diamonds), and ρ Oph (triangles) are distinguished.

Other Images in This Article
Copyright and Terms & Conditions