| Issue |
A&A
Volume 570, October 2014
|
|
|---|---|---|
| Article Number | L14 | |
| Number of page(s) | 6 | |
| Section | Letters | |
| DOI | https://doi.org/10.1051/0004-6361/201425029 | |
| Published online | 03 November 2014 | |
Online material
Maps of the CO(3–2) emission from 36.7 to 53.7 km s-1 at approximately 0.85 km s-1 spectral resolution. As the maps with strong line emission are limited to a dynamic range of ~50 because a significant amount of large scale (> 9′′) flux is not recovered, the rms varies between 30 and 160 mJy in the different velocity channels.
 |
Fig. A.1
CO(3–2) map at 0.9 km s-1 resolution. The crosses mark the positions of Mira A (west) and B (east). Contours are drawn at 3, 5, 10, 20, 40, and 80 times the rms noise level of the respective channel ranging from 30 to 160 mJy. The beam is shown in the lower left corner. |
| Open with DEXTER | |
 |
Fig. A.2
CO(3–2) map averaged from 49 to 54 km s-1. The crosses mark the positions of Mira A (west) and B (east). Contours are drawn at 3, 5, 10, 20, 40, and 80 times the rms noise level of the respective channel ranging from 30 to 160 mJy. The beam is shown in the lower left corner. A spiral is overplotted to clearly mark the spiral windings, and the accretion wake behind the companion is indicated. |
| Open with DEXTER | |
Figure A.2 shows an average from 49 to 54 km s-1 where the spiral windings and the accretion wake discussed in Sects. 3.2 and 4.2 are clearly marked.
© ESO, 2014
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