EDP Sciences
Free Access
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 $\rm {MJy/sr}$ for $\rm 10^{21}H/cm^{2}$. Columns 12-13: emissivity spectral indices in the range 100-240  $\rm ~{\rm\mu m} $ ( $\rm\beta ^{FIR}$) and in the range 550-2100  $\rm ~{\rm\mu m} $ ( $\rm\beta ^{submm}$). Column 14: derived dust temperature in Kelvin. Errors bars represent the 1- $\rm\sigma $ 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 $\rm {MJy/sr}$ for $\rm 10^{21}~H/cm^{2}$. Colums 12-13: emissivity spectral indices in the range 100-240  $\rm ~{\rm\mu m} $ ( $\rm\beta ^{FIR}$) and in the range 550-2100 $\rm ~{\rm\mu m} $ ( $\rm\beta ^{submm}$). Column 14: derived dust temperature in Kelvin. Errors bars represent the 1- $\rm\sigma $ uncertainty estimates. Uncertainties equal to 0.0 are inferior to 0.05.

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