6cm and 11cm polarisation maps of SNR S147 Virtual Observatory Resource

Authors

1. Xiao L.
2. Furst E.
3. Reich W.
4. Han J.L.

Published by

CDS

Abstract

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.

Keywords

1. supernova-remnants
2. radio-sources
3. polarimetry

Bibliographic source Bibcode

2008A&A...482..783X

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/482/783

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/482/783

Document Object Identifer DOI

doi:10.26093/cds/vizier.34820783

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/482/783
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/482/783
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/482/783

IVOA Table Access TAP

http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).