Issue |
A&A
Volume 570, October 2014
|
|
---|---|---|
Article Number | A49 | |
Number of page(s) | 12 | |
Section | Interstellar and circumstellar matter | |
DOI | https://doi.org/10.1051/0004-6361/201424251 | |
Published online | 15 October 2014 |
Online material
Appendix A: Figures
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Fig. A.1
Spectra of CO(4−3) and (3−2), C17O(3−2), SiO(8−7) (multiplied by a factor of five for clarity), SiO(5−4) (blue, where available) and SiO(3−2) (red). The CH3CHO features at 347.35 GHz (Sect. 3) are labelled. |
Open with DEXTER |
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Fig. A.2
Spectra of CO(3−2), C17O(3−2), SiO(8−7) (multiplied by a factor of five for clarity), SiO(5−4) (blue, where available) and SiO(3−2) (red). The CH3CHO features at 347.35 GHz (Sect. 3) are labelled. |
Open with DEXTER |
![]() |
Fig. A.3
Spectra of CO(4−3) and (3−2), C17O(3−2), SiO(8−7) (black), SiO(5−4) (blue, where available) and SiO(3−2) (red) for the three sources not detected in SiO(8−7) (see Table 3). |
Open with DEXTER |
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Fig. A.4
Luminosities of SiO(8−7) a), SiO(3−2) b) and SiO(2−1) c) as a function of their corresponding line width. 22 μ-quiet and 22 μ-loud sources are marked as black and red filled circles. Red stars are 8 μ-loud sources. |
Open with DEXTER |
© ESO, 2014
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