vsini of binaries with evolved component

DOI

In the present study we analyze the behavior of the rotational velocity, vsini, for a large sample of 134 spectroscopic binary systems with a giant star component of luminosity class III, along the spectral region from middle F to middle K.

Cone search capability for table J/ApJ/578/943/table2 (Stellar parameters for binary systems with evolved components)

Identifier
DOI http://doi.org/10.26093/cds/vizier.15780943
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/ApJ/578/943
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/578/943
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/578/943
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/ApJ/578/943
Provenance
Creator de Medeiros J.R.; da Silva J.R.P.; Maia M.R.G.
Publisher CDS
Publication Year 2003
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; Exoplanet Astronomy; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy