Multiphase magnetic fields in the galaxy NGC 3627

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SYSNO ASEP	0583604
Document Type	J - Journal Article
R&D Document Type	Journal Article
Subsidiary J	Článek ve WOS
Title	Multiphase magnetic fields in the galaxy NGC 3627
Author(s)	Liu, M. (US)
Number of authors	5
Source Title	Monthly Notices of the Royal Astronomical Society. - : Oxford University Press - ISSN 0035-8711 Roč. 519, č. 1 (2023), s. 1068-1079
Number of pages	12 s.
Publication form	Online - E
Language	eng - English
Country	US - United States
Keywords	magnetohydrodynamics ; turbulence ; ISM magnetic field
OECD category	Astronomy (including astrophysics,space science)
Research Infrastructure	EU-ARC.CZ III - 90259 - Astronomický ústav AV ČR, v. v. i.
Method of publishing	Limited access
UT WOS	000904994000013
EID SCOPUS	85148992017
DOI	10.1093/mnras/stac3518
Annotation	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.
Workplace	Astronomical Institute
Contact	Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326
Year of Publishing	2024
Electronic address	https://doi.org/10.1093/mnras/stac3518

Number of the records: 1