| Issue |
A&A
Volume 567, July 2014
|
|
|---|---|---|
| Article Number | A10 | |
| Number of page(s) | 9 | |
| Section | Interstellar and circumstellar matter | |
| DOI | https://doi.org/10.1051/0004-6361/201323122 | |
| Published online | 04 July 2014 | |
Online material
Appendix A: 12CO J = 2–1 and 12CO J = 3–2 channel maps as derived from our KOSMA observations in the Swiss Alps
Figures A.1 and A.2 present channel maps for the two molecular line transitions 12CO J = 2−1 and 12CO J = 3−2 integrated over narrow ranges in VLSR. The molecular line data were acquired by the KOSMA 3-m telescope in the Swiss Alps. Detailed descriptions of the observations can be found in Sect. 2.
 |
Fig. A.1
Molecular transition 12CO J = 2−1 channel maps. The center velocities are shown in the upper left corners of each panel in units of km s-1. The integrated velocity interval in each panel is 1.1 km s-1. The contour levels are from 20% up to 90% of the peak with an adjacent contour intervals of 10%. The solid black circle in the lower left corner gives the beam size. |
| Open with DEXTER | |
 |
Fig. A.2
Molecular 12CO J = 3 − 2 channel maps. The center velocities are shown in the upper left corners of each panel in units of km s-1. The integrated velocity interval in each panel is 1.1 km s-1. The contour levels are from 20% up to 90% of the peak with an adjacent 10% contour interval. The solid black circle in the lower left corner gives the beam size. |
| Open with DEXTER | |
© ESO, 2014
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