Free Access
Issue
A&A
Volume 553, May 2013
Article Number A116
Number of page(s) 36
Section Extragalactic astronomy
DOI https://doi.org/10.1051/0004-6361/201321163
Published online 17 May 2013

Online material

Appendix A: Multiwavelenth maps of individual galaxies

thumbnail Fig. A.1

NGC 4178: from top left to bottom right: 6 cm total power emission distribution on DSS B band image together with the apparent B vectors, 20 cm total power emission distribution on DSS B band image together with the apparent B vectors, 6 cm polarized emission distribution, Goldmine Hα emission distribution on spectral index map, and 6 cm polarized emission distribution on degree of polarization. The sizes of the B vectors are proportional to the polarized intensity. Contour levels are ξ × (−3,3,5,8,12,20,30,50,80,120,200,300), with ξ = 12 μJy for the 6 cm total power emission, ξ = 80 μJy for the 20 cm total power emission, and ξ = 12 μJy for the 6 cm polarized emission.

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thumbnail Fig. A.2

NGC 4192: from top left to bottom right: 6 cm total power emission distribution on DSS B band image together with the apparent B vectors, 20 cm total power emission distribution on DSS B band image together with the apparent B vectors, 6 cm polarized emission distribution on VIVA Hi distribution, Goldmine Hα emission distribution on spectral index map, and 6 cm polarized emission distribution on degree of polarization. The sizes of the B vectors are proportional to the polarized intensity. Contour levels are ξ × (−3,3,5,8,12,20,30,50,80,120,200,300), with ξ = 16 μJy for the 6 cm total power emission, ξ = 210 μJy for the 20 cm total power emission, and ξ = 10 μJy for the 6 cm polarized emission.

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thumbnail Fig. A.3

NGC 4216: same panels as in Fig. A.2. Contour levels are ξ × (−3,3,5,8,12,20,30,50,80,120,200,300), with ξ = 9 μJy for the 6 cm total power emission, ξ = 110 μJy for the 20 cm total power emission, and ξ = 7 μJy for the 6 cm polarized emission.

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thumbnail Fig. A.4

NGC 4294: same panels as in Fig. A.2. Contour levels are ξ × (−3,3,5,8,12,20,30,50,80,120,200,300), with ξ = 10 μJy for the 6 cm total power emission, ξ = 200 μJy for the 20 cm total power emission, and ξ = 8 μJy for the 6 cm polarized emission.

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thumbnail Fig. A.5

NGC 4298 (western galaxy): same panels as in Fig. A.2. Contour levels are ξ × (−3,3,5,8,12,20,30,50,80,120,200,300), with ξ = 11 μJy for the 6 cm total power emission, ξ = 170 μJy for the 20 cm total power emission, and ξ = 10 μJy for the 6 cm polarized emission.

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thumbnail Fig. A.6

NGC 4299: same panels as in Fig. A.2. Contour levels are ξ × (−3,3,5,8,12,20,30,50,80,120,200,300), with ξ = 10 μJy for the 6 cm total power emission, ξ = 180 μJy for the 20 cm total power emission, and ξ = 8 μJy for the 6 cm polarized emission.

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thumbnail Fig. A.7

NGC 4303: same panels as in Fig. A.1. Contour levels are ξ × (−3,3,5,8,12,20,30,50,80,120,200,300), with ξ = 30 μJy for the 6 cm total power emission, ξ = 450 μJy for the 20 cm total power emission, and ξ = 12 μJy for the 6 cm polarized emission.

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thumbnail Fig. A.8

NGC 4330: same panels as in Fig. A.2. Contour levels are ξ × (−3,3,5,8,12,20,30,50,80,120,200,300), with ξ = 14 μJy for the 6 cm total power emission, ξ = 210 μJy for the 20 cm total power emission, and ξ = 10 μJy for the 6 cm polarized emission.

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thumbnail Fig. A.9

NGC 4419: same panels as in Fig. A.2. Contour levels are ξ × (−3,3,5,8,12,20,30,50,80,120,200,300), with ξ = 11 μJy for the 6 cm total power emission, ξ = 130 μJy for the 20 cm total power emission, and ξ = 7 μJy for the 6 cm polarized emission.

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thumbnail Fig. A.10

NGC 4424: same panels as in Fig. A.2. Contour levels are ξ × (−3,3,5,8,12,20,30,50,80,120,200,300), with ξ = 14 μJy for the 6 cm total power emission, ξ = 20 μJy for the 20 cm total power emission, and ξ = 7 μJy for the 6 cm polarized emission.

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thumbnail Fig. A.11

NGC 4457: same panels as in Fig. A.2. Contour levels are ξ × (−3,3,5,8,12,20,30,50,80,120,200,300), with ξ = 23 μJy for the 6 cm total power emission, ξ = 190 μJy for the 20 cm total power emission, and ξ = 15 μJy for the 6 cm polarized emission.

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thumbnail Fig. A.12

NGC 4532: same panels as in Fig. A.2. Contour levels are ξ × (−3,3,5,8,12,20,30,50,80,120,200,300), with ξ = 18 μJy for the 6 cm total power emission, ξ = 160 μJy for the 20 cm total power emission, and ξ = 8 μJy for the 6 cm polarized emission.

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thumbnail Fig. A.13

NGC 4567/68: same panels as in Fig. A.2. Contour levels are ξ × (−3,3,5,8,12,20,30,50,80,120,200,300), with ξ = 14 μJy for the 6 cm total power emission, ξ = 230 μJy for the 20 cm total power emission, and ξ = 12 μJy for the 6 cm polarized emission.

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thumbnail Fig. A.14

NGC 4579: same panels as in Fig. A.2. Contour levels are ξ × (−3,3,5,8,12,20,30,50,80,120,200,300), with ξ = 18 μJy for the 6 cm total power emission, ξ = 250 μJy for the 20 cm total power emission, and ξ = 10 μJy for the 6 cm polarized emission.

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thumbnail Fig. A.15

NGC 4689: same panels as in Fig. A.2. Contour levels are ξ × (−3,3,5,8,12,20,30,50,80,120,200,300), with ξ = 14 μJy for the 6 cm total power emission, ξ = 80 μJy for the 20 cm total power emission, and ξ = 12 μJy for the 6 cm polarized emission.

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thumbnail Fig. A.16

NGC 4713: same panels as in Fig. A.2. Contour levels are ξ × (−3,3,5,8,12,20,30,50,80,120,200,300), with ξ = 12 μJy for the 6 cm total power emission, ξ = 120 μJy for the 20 cm total power emission, and ξ = 8 μJy for the 6 cm polarized emission.

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thumbnail Fig. A.17

NGC 4808: same panels as in Fig. A.2. Contour levels are ξ × (−3,3,5,8,12,20,30,50,80,120,200,300), with ξ = 14 μJy for the 6 cm total power emission, ξ = 140 μJy for the 20 cm total power emission, and ξ = 9 μJy for the 6 cm polarized emission.

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© ESO, 2013

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