EH Cnc RV light curves Virtual Observatory Resource

Authors
  1. Yang Y.-G.
  2. Shao Z.-Y.
  3. Pan H.-J.
  4. Yin X.-G.
  5. Published by
    CDS
Abstract

New CCD photometry for the eclipsing binary EH Cnc was made from 2009 to 2011, and five new eclipsing times are presented. Through using the updated Wilson-Devinney code, we first deduced the photometric solution at {chi}^2^=0.9906. The results show that EH Cnc is a W-type contact binary, whose mass ratio and overcontact degree are q=2.51(+/-0.02) and f=27.7%(+/-3.4%) , respectively.

Keywords
  1. eclipsing-binary-stars
  2. photometry
Bibliographic source Bibcode
2011PASP..123..895Y
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/PASP/123/895
IVOA Identifier IVOID
ivo://CDS.VizieR/J/PASP/123/895

Access

Web browser access HTML
https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/PASP/123/895
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/PASP/123/895
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/PASP/123/895
IVOA Table Access TAP
https://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).

History

2014-03-06T15:50:30Z
Resource record created
2014-03-06T15:50:30Z
Created
2017-06-29T08:56:03Z
Updated

Contact

Name
CDS support team
Postal Address
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
E-Mail
cds-question@unistra.fr