Magnetic fields in planetary nebulae detected through non-thermal radio continuum emission
Abstract
Figures and images for the paper accepted in Astronomy & Astrophysics "Magnetic fields in planetary nebulae detected through non-thermal radio continuum emission" by Marcin Hajduk, Timothy Shimwell, Glenn White, Marijke Haverkorn, Jesús A. Toalá, and Ralf-Jürgen Dettmar. The LoTSS DR3 fits images and the catalougue will be published in Shimwell et al.
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Fig. A1. PN radio spectra. Article number, page 1 of 7
A&A proofs: manuscript no. output Fig. A2. PN radio spectra. Article number, page 2 of 7
Fig. A3. PN radio spectra. Article number, page 3 of 7
A&A proofs: manuscript no. output Fig. A4. 144 MHz radio (blue) and optical (orange) emission: Abell 2, Abell 3, Abell 53, AGP 2, IPHASX J022045.0+631134, IPHASX J191255.4+14324, IPHASX J193740.4+203547, IPHASX J221118.0+552841. Article number, page 4 of 7
Fig. A5. 144 MHz radio (blue) and Hα(orange) emission: IRAS 03272+5528, IRAS 19086+0603, K3-91, KK 26, KLSS 1-2, Kn 7, Kn 43, M 1-79. Article number, page 5 of 7
A&A proofs: manuscript no. output Fig. A6. 144 MHz radio (blue) and Hα(orange) emission: NGC 6058 (R band), NGC 6742 (R band), NGC 6781, NGC 6894, NGC 6842, PaEk 1, PM 1-20, PM 1-305. Article number, page 6 of 7
Fig. A7. 144 MHz radio (blue) and Hα(orange) emission: PM 1-333, Pre 21 (B band), Ra50, TaWe2, Te5, WeSb4. Article number, page 7 of 7