EDP Sciences
Free Access
Volume 534, October 2011
Article Number A56
Number of page(s) 12
Section Extragalactic astronomy
DOI https://doi.org/10.1051/0004-6361/201117533
Published online 03 October 2011

Online material

Appendix A: Additional figures

thumbnail Fig. A.1

Continuum maps at 23.7 GHz for IC 342 (left), Maffei 2 (middle), and NGC 253 (right). The contour levels are, −0.3, 0.3, 0.6, 1.2, 2.4, 4.8 mJy beam-1 for IC 342, −0.6, 0.6, 1.2, 2.4, 4.8 mJy beam-1 for Maffei 2, and −2.7, 2.7, 5.4, 10.8, 21.6, 43.2, 86.4 mJy beam-1 for NGC 253. The beams are shown at the bottom left corner of each map.

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thumbnail Fig. A.2

Channel maps of the NH3(1, 1) and NH3(2, 2) transition emission from IC 342. The contour levels are −0.9, 0.9, 1.8, 2.7, and 3.6 mJy beam-1 and −0.75, 0.75, 1.5, 2.25, and 3 mJy beam-1, respectively. The synthesized beams are shown in the lower left corner of the first panel for each transition. The gray scale images represent the continuum emission at 23.7 GHz.

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thumbnail Fig. A.3

Channel maps of the NH3(1, 1) and NH3(2, 2) emission from Maffei 2. The contour levels are −0.78, 0.78, 1.56, 2.34, and 3.12 mJy beam-1 and −1.2, 1.2, 2.4, 3.6, and 4.8 mJy beam-1, respectively. The gray scale images show the continuum emission at 23.7 GHz. Beams are shown in the left upper panel for each map set.

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thumbnail Fig. A.4

Channel maps of the NH3(3, 3) transition from NGC 253. The contour levels are −1.8, 1.8, 3.6, 5.4, 7.2, and 9.0 mJy beam-1. The synthesized beam is shown in the left lower corner in the first panel. The gray scale images represent the continuum emission at 23.7 GHz.

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© ESO, 2011

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