Issue |
A&A
Volume 506, Number 2, November I 2009
|
|
---|---|---|
Page(s) | 745 - 756 | |
Section | Interstellar and circumstellar matter | |
DOI | https://doi.org/10.1051/0004-6361/200811246 | |
Published online | 18 August 2009 |
Online Material
Appendix: A
Table 7: Results of the IR/HI correlations in the atomic phase for all sky regions. Cols. 1-2: central position of each studied regions in degree. Column 3: number of pixels used for the correlations in each studied regions. Columns 4-11: results of the correlations in for . Columns 12-13: emissivity spectral indices in the range 100-240 ( ) and in the range 550-2100 ( ). Column 14: derived dust temperature in Kelvin. Errors bars represent the 1- uncertainty estimates.
Table 8: Results of the IR/CO correlations in the molecular phase for all sky regions. Columns 1-2: central position of each studied regions in degree. Column 3: number of pixels used for the correlations in each studied regions. Columns 4-11: results of the correlations in for . Colums 12-13: emissivity spectral indices in the range 100-240 ( ) and in the range 550-2100 ( ). Column 14: derived dust temperature in Kelvin. Errors bars represent the 1- uncertainty estimates. Uncertainties equal to 0.0 are inferior to 0.05.
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