Stars observed with Doppler imaging

Starspots are created by local magnetic fields on the surfaces of stars, just as sunspots. Their fields are strong enough to suppress the overturning convective motion and thus block or redirect the flow of energy from the stellar interior outwards to the surface and consequently appear as locally cool and therefore dark regions against an otherwise bright photosphere. This article is an attempt to review our current knowledge of starspots.

Cone search capability for table J/other/A+ARV/17.251/table1 (Late-type stars with Doppler images (as of 2008))

Identifier
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/other/A+ARV/17.251
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/other/A+ARV/17.251
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/other/A+ARV/17.251
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/other/A+ARV/17.251
Provenance
Creator Strassmeier K.G.
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