Multiphase magnetic fields in the galaxy NGC 3627
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A90259%2F23%3A00583604" target="_blank" >RIV/67985815:90259/23:00583604 - isvavai.cz</a>
Result on the web
<a href="https://doi.org/10.1093/mnras/stac3518" target="_blank" >https://doi.org/10.1093/mnras/stac3518</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1093/mnras/stac3518" target="_blank" >10.1093/mnras/stac3518</a>
Alternative languages
Result language
angličtina
Original language name
Multiphase magnetic fields in the galaxy NGC 3627
Original language description
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.
Czech name
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Czech description
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Classification
Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
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OECD FORD branch
10308 - Astronomy (including astrophysics,space science)
Result continuities
Project
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Continuities
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Others
Publication year
2023
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Monthly Notices of the Royal Astronomical Society
ISSN
0035-8711
e-ISSN
1365-2966
Volume of the periodical
519
Issue of the periodical within the volume
1
Country of publishing house
US - UNITED STATES
Number of pages
12
Pages from-to
1068-1079
UT code for WoS article
000904994000013
EID of the result in the Scopus database
2-s2.0-85148992017