The geometry of the magnetic field in the central molecular zone measured by PILOT

Simple item page
dc.contributor.authorMangilli, A.
dc.contributor.authorAlsalloum, Mohammad A.
dc.contributor.authorAlmuqbil, Fatimah A.
dc.contributor.authorAlhowais, Nayef A.
dc.contributor.authorAlhassun, Ahmed M.
dc.date.accessioned2025-08-19T04:27:56Z
dc.date.available2025-08-19T04:27:56Z
dc.date.issued2018-11-01
dc.description.abstractThe study reports on the magnetic field geometry in the Central Molecular Zone (CMZ) of the Milky Way as observed by the balloon-borne submillimeter polarimeter PILOT. The results reveal that the magnetic field in the CMZ is largely organized and aligned with the Galactic plane, providing constraints on gas dynamics, star formation processes, and the role of magnetic fields in the inner Galaxy.en
dc.identifier.citationMangilli, A.; et al. (2018). The geometry of the magnetic field ... A&A 618, A86. DOI: 10.1051/0004-6361/201832844en
dc.identifier.doi10.1051/0004-6361/201832844
dc.identifier.otherFilename:85082393183_The geometry of the magnetic field in the central molecular zone measured by PIL.pdf
dc.identifier.urihttps://doi.org/10.1051/0004-6361/201832844
dc.identifier.urihttps://nur.nu.edu.kz/handle/123456789/9427
dc.language.isoen
dc.publisherEDP Sciences
dc.relation.ispartofAstronomy & Astrophysics, 618, A86en
dc.sourceAstronomy & Astrophysics, 618, A86 (2018)en
dc.subjectGalactic center Magnetic fields Polarization Interstellar medium Submillimeter astronomy en
dc.titleThe geometry of the magnetic field in the central molecular zone measured by PILOTen
dc.typeJournal Articleen

Files

Original bundle

Now showing 1 - 1 of 1
Thumbnail Image
Name:
85082393183_The geometry of the magnetic field in the central molecular zone measured by PIL.pdf
Size:
14.26 MB
Format:
Adobe Portable Document Format
Download

Collections

Articles