Image Details

Choose export citation format:

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. 1.

Contours of constant ﹩\chi ^{2}_{\nu }﹩ value (the goodness‐of‐fit) over the parameter space spanned by the beam‐filling factor (ηbf) and column density (N) (left panel), and by the rotation temperature and column density (right panel). A cross marks the best‐fit parameters (giving the smallest ﹩\chi ^{2}_{\nu }﹩) in each of the panels. In the left panel the rotation temperature is not a free parameter, but is fixed at 182 K, and because of this the confidence regions are only approximate.

Other Images in This Article

Show More

Copyright and Terms & Conditions