| Issue |
A&A
Volume 536, December 2011
|
|
|---|---|---|
| Article Number | A33 | |
| Number of page(s) | 23 | |
| Section | Interstellar and circumstellar matter | |
| DOI | https://doi.org/10.1051/0004-6361/201117112 | |
| Published online | 05 December 2011 | |
Online material
Appendix A: Full spectral range
In Figs. A.1−A.3, we show the full observed spectral range, convolved to a resolution of 5′′, and label the identified lines with the molecule (see also Sect. 3.2).
 |
Fig. A.1
Full spectral range towards G10.47+0.03 convolved to 5′′ resolution. The green overlay is the myXLASS model for all molecules except HC3N, whose emission is overlaid in red. The displayed panels cover 199.85–201.85 GHz (upper three) and 209.85–210.55 GHz (bottom); the rest is shown in Figs. A.2 and A.3. |
| Open with DEXTER | |
 |
Fig. A.2
As in Fig. A.1, displaying 210.5–211.85 GHz (upper two) and 344.05–345.95 GHz (lower two). |
| Open with DEXTER | |
 |
Fig. A.3
As in Fig. A.1, displaying 354.1–355.95 GHz (upper two), 680.2–682.3 GHz (third panel from top), and 690.2–692.3 GHz (bottom). |
| Open with DEXTER | |
Appendix B: Line maps
In Fig. B.1 we show 100 integrated line maps, ordered by molecule as in Table 3 and by frequency of the transition (see also Sect. 3.3).
 |
Fig. B.1
Integrated line maps. Above each panel, the molecule, the frequency of the transition (in GHz), and the velocity range (in km s-1) are given. The map size is either 5, 10, or 15′′, as written in the map (tick spaces are 1′′, centered on RA 18:08:38.236, Dec –19:51:50.25). Beams are shown in the lower left, and the number in the lower right of each panel is the maximum flux in K km s-1 (the contours are ± 20 and 50% of that value). The color scale ranges from the minimum to the maximum value. The energy of the lower level is given in the upper left. |
| Open with DEXTER | |
 |
Fig. B.1
continued. |
| Open with DEXTER | |
 |
Fig. B.1
continued. |
| Open with DEXTER | |
 |
Fig. B.1
continued. |
| Open with DEXTER | |
 |
Fig. B.1
continued. |
| Open with DEXTER | |
© ESO, 2011
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