Multiphase magnetic fields in the galaxy NGC 3627

0583604 - ASÚ 2024 RIV US eng J - Journal Article
Liu, M. … Total 5 authors
Multiphase magnetic fields in the galaxy NGC 3627.
Monthly Notices of the Royal Astronomical Society. Roč. 519, č. 1 (2023), s. 1068-1079. ISSN 0035-8711. E-ISSN 1365-2966
Research Infrastructure: EU-ARC.CZ III - 90259
Keywords : magnetohydrodynamics * turbulence * ISM magnetic field
OECD category: Astronomy (including astrophysics,space science)
Impact factor: 4.8, year: 2022
Method of publishing: Limited access
https://doi.org/10.1093/mnras/stac3518

We study the Seyfert galaxy NGC 3627's magnetic field orientations measured from the synchrotron polarization observed with the Very Large Array and from the Velocity Gradient Technique (VGT) using spectroscopic data. The latter employs the magnetohydrodynamical turbulence's anisotropy to probe the magnetic fields. Being applied to the CO (2-1) and H α emission lines obtained from the PHANGS-ALMA and PHANGS-MUSE surveys, it reveals the magnetic field orientation globally consistent with the polarization.
Permanent Link: https://hdl.handle.net/11104/0351613