| Issue |
A&A
Volume 568, August 2014
|
|
|---|---|---|
| Article Number | L5 | |
| Number of page(s) | 5 | |
| Section | Letters | |
| DOI | https://doi.org/10.1051/0004-6361/201424103 | |
| Published online | 14 August 2014 | |
Online material
Appendix A: C17O, C34S, and CH3OH kinematics
We report in Figs. A.1 and A.2 the channel maps of the C17O(3–2) and C34S(7–6) (continuum-subtracted) emissions towards HH212 that were analysed and discussed in the main text.
 |
Fig. A.1
Channel maps of the C17O(3–2) (continuum-subtracted) emissions towards HH212. The bottom-right panel shows in magenta the 0.43 km s-1 wide channel (centred on +1.13 km s-1) where emission is most spatially extended. The other panels superposed in blue and red contours are the channel maps at symmetric blue/red velocity offsets from this central channel, with the velocity shift given (in km s-1) in the upper-right corner. The black cross (inclined to show the SiO jet direction) indicates the position of the MM1 continuum source. The ellipse in the top-left panel shows the ALMA synthesised beam (HPBW): |
| Open with DEXTER | |
 |
Fig. A.2
Channel maps of the C34S(7–6) blue- and redshifted (continuum-subtracted) emissions towards HH212. The bottom-right panel shows in magenta the 0.43 km s-1 wide channel (centred on +1.42 km s-1) where emission is the most spatially extended. The other panels superposed in blue and red contours are the channel maps at symmetric blue and red velocity offsets from this central channel, with the velocity shift given (in km s-1) in the upper-right corner. Symbols are the same as in Fig. A.1. First contours and steps correspond to 5σ (15 mJy beam-1 km s-1). |
| Open with DEXTER | |
© ESO, 2014
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