vsini of B0-B3 stars in 7 young clusters

DOI

We present the results of a study aimed at assessing the differences in the distribution of rotation speeds N(vsini) among young (1-15Myr) B stars spanning a range of masses 6M_{sun}<M<12M{sun} and located in different environments: seven low-density ({rho}>1M{sun}_/pc^3^) ensembles that will survive as rich, bound stellar clusters for ages well in excess of 10^8^yr.

Cone search capability for table J/AJ/133/1092/table1 (Stellar Data)

Cone search capability for table J/AJ/133/1092/table2 (Data for Stellar Associations)

Identifier
DOI http://doi.org/10.26093/cds/vizier.51331092
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/AJ/133/1092
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/133/1092
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/133/1092
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/AJ/133/1092
Provenance
Creator Wolff S.C.; Strom S.E.; Dror D.; Venn K.
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; Physics; Stellar Astronomy