Low-mass binary companions in M35

DOI

The Hubble Space Telescope Fine Guidance Sensors data on 23 stars in the intermediate-age cluster M35 having B-V6AU, secondary masses between 0.3 and 0.6M_{sun}_, and mass ratios of about 0.2. This latter value is in agreement with capture models employing stars with circumstellar disks for the formation of binaries.

Cone search capability for table J/AJ/133/394/table2 (HST FGS Observations of M35 Stars in the POS Mode)

Identifier
DOI http://doi.org/10.26093/cds/vizier.51330394
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/AJ/133/394
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/133/394
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/133/394
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/AJ/133/394
Provenance
Creator McNamara B.J.; Harrison T.E.; McArthur B.
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