High-resolution radio continuum survey of M 33

2008/09/02 by F. S. Tabatabaei, M. Krause, Andrew Fletcher +2 · 81 citations
Physics and Astronomy · #Astronomy #Astrophysical Phenomena and Observations #Astrophysics #Astrophysics and Cosmic Phenomena #Galaxies: Formation, Evolution, Phenomena #Galaxy #Physics #astro-ph

paper · pdf · doi:10.1051/0004-6361:200810590

published in Astronomy and Astrophysics 490(3), 1005-1017 (EDP Sciences) · 17 pages, 12 figures, accepted for Astronomy and Astrophysics publication

arxiv created 2008/09/02 · openalex publication_date 2008/09/23 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Aims. We study the magnetic field structure, strength, and energy density in the Scd galaxy M 33.

Citations

• The interstellar environment of our galaxy
• Revised equipartition and minimum energy formula for magnetic field strength estimates from radio synchrotron observations
• The Three-Phase Interstellar Medium Revisited

Cited by

• Multi-scale radio-infrared correlations in M 31 and M 33: The role of magnetic fields and star formation
• Magnetic fields in the nearby spiral galaxy IC 342: A multi-frequency radio polarization study
• Modeling the total and polarized emission in evolving galaxies: “Spotty” magnetic structures
• Nonthermal Emission from Star-Forming Galaxies