| Issue |
A&A
Volume 526, February 2011
|
|
|---|---|---|
| Article Number | A9 | |
| Number of page(s) | 16 | |
| Section | Interstellar and circumstellar matter | |
| DOI | https://doi.org/10.1051/0004-6361/201015319 | |
| Published online | 14 December 2010 | |
Online material
Appendix A: Figures
 |
Fig. A.1
Most interesting frames from the RM-cube. The contour levels are 3, 6, 12, 24,...mJy beam-1 rmtf-1 (1.4, 2.8, 5.5, ... K rmtf-1). The Faraday depth in rad m-2 is indicated in the top left corner of each frame. The HPBW is 2′ × 3′. |
| Open with DEXTER | |
 |
Fig. A.1
continued. |
| Open with DEXTER | |
 |
Fig. A.1
continued. |
| Open with DEXTER | |
 |
Fig. A.1
continued. |
| Open with DEXTER | |
 |
Fig. A.2
Polarization vectors (electric field) at 350.22 MHz overlaid on contour maps of the absolute value of the Faraday dispersion function. Contours are drawn at +3, +6 , +12, etc. mJy beam-1 rmtf-1. The polarization vectors are drawn if |F(φ)| is larger than 5 times the local observed RMS at |φ| > 100 rad m-2. The Faraday depth in rad m-2 is plotted in the top left corner of each image. |
| Open with DEXTER | |
 |
Fig. A.2
continued. |
| Open with DEXTER | |
© ESO, 2010
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