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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