BD+20 1790 radial velocity curve

The young active star BD +20 1790 has been inferred to host a substellar companion from radial-velocity measurements that detected the reflex motion induced on the parent star. We attempt to completely characterize the radial-velocity signal in order to assess its nature.

Identifier
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/513/L8
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/513/L8
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/513/L8
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/513/L8
Provenance
Creator Figueira P.; Marmier M.; Bonfils X.; Di Folco E.; Udry S.; Santos N.C.,Lovis C.; Megevand D.; Melo C.H.F.; Pepe F.; Queloz D.; Segransan D.,Triaud A.H.M.J.; Viana Almeida P.
Publisher CDS
Publication Year 2010
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