vsini of Orion low-mass stars

DOI

Projected rotational velocities (vsini) have been measured for a sample of 145 stars with masses between 0.4 and greater than 10M_{sun} (median mass 2.1M{sun}) located in the Orion star-forming complex. These measurements have been supplemented with data from the literature for Orion stars with masses as low as 0.1M{sun}_.

Cone search capability for table J/ApJ/601/979/rot (Observed and Derived parameters)

Identifier
DOI http://doi.org/10.26093/cds/vizier.16010979
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/ApJ/601/979
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/601/979
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/601/979
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/ApJ/601/979
Provenance
Creator Wolff S.C.; Strom S.E.; Hillenbrand L.A.
Publisher CDS
Publication Year 2009
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