Magnetic fields in white dwarfs

DOI

A large number of magnetic white dwarfs discovered in the SDSS have so far only been analyzed by visual comparison of the observations with relatively simple models of the radiation transport in a magnetised stellar atmosphere. We model the structure of the surface magnetic fields of the hydrogen-rich white dwarfs in the SDSS.

Cone search capability for table J/A+A/506/1341/table3 (Model fits with centered dipole and offset dipole models with comparison to literature values)

Identifier
DOI http://doi.org/10.26093/cds/vizier.35061341
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/506/1341
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/506/1341
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/506/1341
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/506/1341
Provenance
Creator Kuelebi B.; Jordan S.; Euchner F.; Gaensicke B.T.; Hirsch H.
Publisher CDS
Publication Year 2010
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; Observational Astronomy; Physics; Stellar Astronomy