Evolutionary state of magnetic CP stars

DOI

The photospheres of about 5-10% of the upper main sequence stars exhibit remarkable chemical anomalies. Many of these chemically peculiar (CP) stars have a global magnetic field, the origin of which is still a matter of debate. We present a comprehensive statistical investigation of the evolution of magnetic CP stars, aimed at providing constraints to the theories that deal with the origin of the magnetic field in these stars.

Cone search capability for table J/A+A/450/763/table1 ( measurements for the sample of CP stars observed with FORS1 (data retrieved from the ESO archive))

Cone search capability for table J/A+A/450/763/table2 (Fundamental parameters of magnetic CP stars)

Identifier
DOI http://doi.org/10.26093/cds/vizier.34500763
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/450/763
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/450/763
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/450/763
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/450/763
Provenance
Creator Kochukhov O.; Bagnulo S.
Publisher CDS
Publication Year 2007
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; Natural Sciences; Physics; Stellar Astronomy