Wilson-Bappu relation in late-type stars Virtual Observatory Resource

Authors

1. Pace G.
2. Pasquini L.
3. Ortolani S.

Published by

CDS

Abstract

Wilson & Bappu (1957ApJ...125..661W) have shown the existence of a remarkable correlation between the width of the emission in the core of the K line of CaII and the absolute visual magnitude of late-type stars. Here we present a new calibration of the Wilson-Bappu effect based on a sample of 119 nearby stars. We use, for the first time, width measurements based on high resolution and high signal to noise ratio CCD spectra and absolute visual magnitudes from the Hipparcos database.

Keywords

1. late-type-stars
2. line-intensities

Bibliographic source Bibcode

2003A&A...401..997P

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/401/997

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/401/997

Document Object Identifer DOI

doi:10.26093/cds/vizier.34010997

Access

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http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/401/997
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/401/997
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/401/997

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For use with a cone search client (e.g., TOPCAT).
http://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/401/997/table1?
https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/401/997/table1?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/401/997/table1?