CaII and MgII excess flux density in cool stars

DOI

The relation between the CaII H and K line-tore flux density and rotation period is studied for a sample of 313 cool stars of luminosity classes ranging from II-III to V, and compared to similar relations for MgII h and k and soft X-ray.

Cone search capability for table J/A+A/177/131/table2 (Sample of stars used in the determination of the rotation-activity relation)

Identifier
DOI http://doi.org/10.26093/cds/vizier.31770131
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/177/131
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/177/131
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/177/131
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/177/131
Provenance
Creator Rutten R.G.M.
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 Astrophysics and Astronomy; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy