File:Aa36481-19.pdf
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[edit]DescriptionAa36481-19.pdf |
Abstract
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Date | |
Source | https://www.aanda.org/articles/aa/pdf/2020/01/aa36481-19.pdf |
Author | R. Beck, E. M. Berkhuijsen, R. Gießübel, and D. D. Mulcahy |
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Open Access funding provided by Max Planck Society. |
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current | 21:52, 4 June 2020 | 1,239 × 1,752, 17 pages (2.84 MB) | Fabian RRRR (talk | contribs) | {{Information |description='''Abstract''' * Context. Magnetic fields play an important role in the dynamics and evolution of galaxies; however, the amplification and ordering of the initial seed fields are not fully understood. The nearby spiral galaxy M 31 is an ideal laboratory for extensive studies of magnetic fields. * Aims. Our aim was to measure the intrinsic structure of the magnetic fields in M 31 and compare them with dynamo models of field amplification. * Methods. The intensity... |
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Short title | Magnetic fields and cosmic rays in M 31 - I. Spectral indices, scale lengths, Faraday rotation, and magnetic field pattern |
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Image title | A\&A 633, A5 (2020). DOI: 10.1051/0004-6361/201936481 |
Author | Beck R., Berkhuijsen E. M., Gießübel R., Mulcahy D. D. |
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Software used | LaTeX with hyperref package |
Conversion program | pdfTeX-1.40.14 |
Encrypted | no |
Page size | 595.276 x 841.89 pts (A4) |
Version of PDF format | 1.5 |
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