6cm and 11cm polarisation maps of SNR S147

DOI

S147 is a large faint shell-type supernova remnant (SNR) known for its remarkable spectral break at cm-wavelength, which is an important physical property to characterize SNR evolution. However, the spectral break is based on radio observations with limited precision. New sensitive observations at high frequencies are required for a detailed study of the spectral properties and the magnetic field structure of S147.

Identifier
DOI http://doi.org/10.26093/cds/vizier.34820783
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/482/783
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/482/783
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/482/783
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/482/783
Provenance
Creator Xiao L.; Furst E.; Reich W.; Han J.L.
Publisher CDS
Publication Year 2008
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; Interstellar medium; Natural Sciences; Observational Astronomy; Physics