How to constrain your M dwarf. II. Nearby binaries

DOI

The mass-luminosity relation for late-type stars has long been a critical tool for estimating stellar masses. However, there is growing need for both a higher-precision relation and a better understanding of systematic effects (e.g., metallicity). Here we present an empirical relationship between M_Ks_ and M_* spanning 0.075M{sun}_

Identifier
DOI http://doi.org/10.26093/cds/vizier.18710063
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/ApJ/871/63
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/871/63
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/871/63
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/ApJ/871/63
Provenance
Creator Mann A.W.; Dupuy T.; Kraus A.L.; Gaidos E.; Ansdell M.; Ireland M.,Rizzuto A.C.; Hung C.-L.; Dittmann J.; Factor S.; Feiden G.; Martinez R.A.,Ruiz-rodriguez D.; Chia Thao P.
Publisher CDS
Publication Year 2020
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; Interdisciplinary Astronomy; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy