Issue |
A&A
Volume 529, May 2011
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Article Number | A41 | |
Number of page(s) | 16 | |
Section | Interstellar and circumstellar matter | |
DOI | https://doi.org/10.1051/0004-6361/201016271 | |
Published online | 29 March 2011 |
Online material
Appendix A: KOSMA 12CO 2–1 and 12CO 3–2 imaging of the W43 molecular cloud complex
Fig. A.1
12CO 2–1 intensity map of the inner part of the W43 molecular complex obtained with KOSMA. The lines are integrated over the 80−110 km s-1 velocity range. Contours go from to 40 to 140 by 20 in unit of K km s-1. The HPBW is plotted in the bottom-left corner. |
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Open with DEXTER |
Fig. A.2
12CO 3–2 intensity map of the inner part of the W43 molecular complex obtained with KOSMA. The lines are integrated over the 80−110 km s-1 velocity range. Contours go from to 40 to 140 by 20 in unit of K km s-1. The HPBW is plotted in the bottom-left corner. |
|
Open with DEXTER |
Fig. A.3
Velocity maps of the inner part of the W43 molecular complex in the 12CO 2–1 emission obtained with KOSMA, integrated over ~2 km s-1-wide channels ranging from VLSR = 66 to 118 km s-1. The W43-main and W43-south regions are indicated with white circles. The main molecular bridge linking them is outlined by a dashed curve. The HPBW is plotted in the top-left corner. |
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Open with DEXTER |
Fig. A.4
Velocity maps of the inner part of the W43 molecular complex in the 12CO 3–2 emission obtained with KOSMA, integrated over ~2 km s-1-wide channels ranging from VLSR = 66 to 118 km s-1. The W43-main and W43-south regions are indicated with white circles. The main molecular bridge linking them is outlined by a dashed curve. The HPBW is plotted in the top-left corner. |
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Open with DEXTER |
© ESO, 2011
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