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Submillimetre observations of the two-component magnetic field in M82

Pattle, K; Gear, W; Redman, M; Smith, MWL; Greaves, J; (2021) Submillimetre observations of the two-component magnetic field in M82. Monthly Notices of the Royal Astronomical Society , 505 (1) pp. 684-688. 10.1093/mnras/stab1300. Green open access

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Abstract

We observed the starburst galaxy M82 in 850 µm polarized light with the POL-2 polarimeter on the James Clerk Maxwell Telescope (JCMT). We interpret our observed polarization geometry as tracing a two-component magnetic field: a poloidal component aligned with the galactic ‘superwind’, extending to a height ∼350 pc above and below the central bar; and a spiral-arm-aligned, or possibly toroidal, component in the plane of the galaxy, which dominates the 850 µm polarized light distribution at galactocentric radii ≳2 kpc. Comparison of our results with recent High-resolution Airborne Wideband Camera Plus (HAWC+) measurements of the field in the dust entrained by the M82 superwind suggests that the superwind breaks out from the central starburst at ∼350 pc above the plane of the galaxy.

Type: Article
Title: Submillimetre observations of the two-component magnetic field in M82
Open access status: An open access version is available from UCL Discovery
DOI: 10.1093/mnras/stab1300
Publisher version: https://doi.org/10.1093/mnras/stab1300
Language: English
Additional information: This version is the version of record. For information on re-use, please refer to the publisher’s terms and conditions.
Keywords: galaxies: individual: M82, galaxies: magnetic fields, submillimetre: galaxies
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy
URI: https://discovery.ucl.ac.uk/id/eprint/10137339
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