Brightness and diameters for extragalactic SNRs

DOI

This paper examines relations between the radio surface brightness Sigma and the diameter D (also known as Sigma-D relations) for a sample of extragalactic supernova remnants (SNRs) as constructed from a combination of published data and data from our own surveys. Our sample of extragalactic SNRs is the largest ever devised for the purpose of analyzing Sigma-D relations.

Cone search capability for table J/A+A/435/437/tablea1 (The basic quantities for 148 SNRs in nearby galaxies used for deriving of the updated {Sigma}-D relations.)

Identifier
DOI http://doi.org/10.26093/cds/vizier.34350437
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/435/437
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/435/437
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/435/437
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/435/437
Provenance
Creator Urosevic D.; Pannuti T.G.; Duric N.; Theodorou A.
Publisher CDS
Publication Year 2006
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; Galactic and extragalactic Astronomy; Interstellar medium; Natural Sciences; Physics