IC 342 multi-frequency radio polarization study

DOI

Magnetic fields play an important role in the formation and stabilization of spiral structures in galaxies, but the interaction between interstellar gas and magnetic fields has not yet been understood. In particular, the phenomenon of "magnetic arms" located between material arms is a mystery. The strength and structure of interstellar magnetic fields and their relation to spiral arms in gas and dust are investigated in the nearby and almost face-on spiral galaxy IC 342.

Cone search capability for table J/A+A/578/A93/list (List of fits images)

Associated data

Identifier
DOI http://doi.org/10.26093/cds/vizier.35780093
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/578/A93
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/578/A93
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/578/A93
Related Identifier https://cdsarc.cds.unistra.fr/assocdata/?obs_collection=J/A+A/578/A93
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/578/A93
Provenance
Creator Beck R.
Publisher CDS
Publication Year 2015
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysical Processes; Astrophysics and Astronomy; Cosmology; Galactic and extragalactic Astronomy; Natural Sciences; Physics