Abundances of TX UMa

DOI

High-resolution echelle spectra have been obtained of the semi-detached Algol-type eclipsing binary system, TX UMa with the high-resolution echelle spectrographs of the 1.8m telescope at Bohyunsan Optical Astronomy Observatory in Korea and of the 2.0m telescope of Peak Terskol Observatory in Russia. New accurate radial velocities of its components have been measured.

Identifier
DOI http://doi.org/10.26093/cds/vizier.74152238
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/MNRAS/415/2238
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/415/2238
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/MNRAS/415/2238
Provenance
Creator Glazunova L.V.; Mkrtichian D.E.; Rostopchin S.I.
Publisher CDS
Publication Year 2012
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; Physics; Stellar Astronomy