Issue |
A&A
Volume 504, Number 3, September IV 2009
|
|
---|---|---|
Page(s) | 853 - 867 | |
Section | Interstellar and circumstellar matter | |
DOI | https://doi.org/10.1051/0004-6361/200811257 | |
Published online | 16 July 2009 |
Online Material
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Figure 14: Normalized emission of CS, H2S, OCS, SO, SO2 (and isotopic species) lines from W43MM1. Spectra velocity resolutions are 0.10-0.19 km s-1. The dashed line shows the source LSR velocity. |
Open with DEXTER |
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Figure 15: Normalized emission of CS, H2S, OCS, SO, SO2 (and isotopic species) lines from IRAS18264-1152. Spectra velocity resolutions are 0.10-0.19 km s-1. The dashed line shows the source LSR velocity. |
Open with DEXTER |
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Figure 16: Normalized emission of CS, H2S, OCS, SO, SO2 (and isotopic species) lines from IRAS05358+3543. Spectra velocity resolutions are 0.10-0.19 km s-1. The dashed line shows the source LSR velocity. |
Open with DEXTER |
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Figure 17: Normalized emission of CS, H2S, OCS, SO, SO2 (and isotopic species) lines from IRAS18162-2048. Spectra velocity resolutions are 0.10-0.19 km s-1. The dashed line shows the source LSR velocity. |
Open with DEXTER |
Table 6: Observed line emissions parameters for W43MM1.
Table 7: Observed line emissions parameters for IRAS18264-1152.
Table 8: Observed line emissions parameters for IRAS05358+3543.
Table 9: Observed line emissions parameters for IRAS18162-2048.
Table 10: Opacities derived from modeling the molecular emission of the sources, where ``ND'' stands for no data.
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