RM Synthesis of 33 sources around M31

DOI

Low-frequency radio continuum observations are best suited to search for radio halos of inclined galaxies. Polarization measurements at low frequencies allow the detection of small Faraday rotation measures caused by regular magnetic fields in galaxies and in the foreground of the Milky Way. The detection of low-frequency polarized emission from a spiral galaxy such as M31 allows us to assess the degree of Faraday depolarization, which can be compared with models of the magnetized interstellar medium.

Cone search capability for table J/A+A/559/A27/objects (Source positions and names)

Identifier
DOI http://doi.org/10.26093/cds/vizier.35590027
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/559/A27
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/559/A27
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/559/A27
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/559/A27
Provenance
Creator Giessubel R.; Heald G.; Beck R.; Arshakian T.G.
Publisher CDS
Publication Year 2013
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 Astrophysics and Astronomy; Cosmology; Exoplanet Astronomy; Galactic and extragalactic Astronomy; Natural Sciences; Observational Astronomy; Physics