Fig. 2 from A Three‐Position Spectral Line Survey of Sagittarius B2 between 218 and 263 GHz. II. Data Analysis

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A Three‐Position Spectral Line Survey of Sagittarius B2 between 218 and 263 GHz. II. Data Analysis

Authors: A. Nummelin, P. Bergman, Å. Hjalmarson, P. Friberg, W. M. Irvine, T. J. Millar, M. Ohishi, and S. Saito

Nummelin et al. 2000 The Astrophysical Journal Supplement Series 128 213.

Provider: AAS Journals

Caption: Fig. 2.

In these rotation diagrams the observed line intensities are plotted (circles) together with the intensities resulting from the best‐fit model (triangles). The error bars indicate 30% pointing and calibration uncertainty. Transitions suspected to be significantly blended with other species have been excluded.

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