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Analysis of spiral arms using anisotropic wavelets: gas, dust and magnetic fields in M 51

2006/08/25 by I. Patrikeev, A. Fletcher, Andrew Fletcher +7 · 1 citation
Mathematics · Physics and Astronomy · #Anisotropy #Artificial intelligence #Astrophysics #Astrophysics and Star Formation Studies #Computer science #Context (archaeology) #Galaxies: Formation, Evolution, Phenomena #Galaxy #Geology #Magnetic field #Mathematical analysis #Mathematics #Optics #Physics #Quantum mechanics #Spiral (railway) #Spiral galaxy #Stellar, planetary, and galactic studies #Wavelet #astro-ph

paper · pdf · doi:10.1051/0004-6361:20065225

13 pages, 10 figures (2 in colour), accepted for publication in Astronomy and Astrophysics

openalex publication_date 2006/08/25 · arxiv created 2006/09/28 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

Context.The origin of the spiral pattern of magnetic fields in disc galaxies is an open question.

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