Eclipsing binary HU Tauri Virtual Observatory Resource

Authors

1. Parthasarathy M.
2. Sarma M.B.K.
3. Vivekananda Rao P.

Published by

CDS

Abstract

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.

Keywords

1. eclipsing-binary-stars
2. photometry

Bibliographic source Bibcode

1995A&A...297..359P

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/297/359

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/297/359

Document Object Identifer DOI

doi:10.26093/cds/vizier.32970359

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/297/359
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/297/359
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/297/359

IVOA Table Access TAP

http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).