Fig. 3 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. 3.

H₂ column density as a function of angular resolution for Sgr B2(N) and Sgr B2(M), respectively. Observed values (Table 4) have been indicated with squares. The curves were calculated by convolving the density distribution (eq. [14]) with a Gaussian corresponding to the angular resolution

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