Eclipsing binary HU Tauri

DOI

The photometric elements of HU Tauri are derived from an analysis of its blue and visual light curves using the Wilson and Devinney (1971, ApJ 166, 605) light curve synthesis method. Combining the photometric elements and spectroscopic orbital elements the absolute dimensions of the system are derived.

Identifier
DOI http://doi.org/10.26093/cds/vizier.32970359
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/297/359
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/297/359
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/297/359
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/297/359
Provenance
Creator Parthasarathy M.; Sarma M.B.K.; Vivekananda Rao P.
Publisher CDS
Publication Year 1997
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