BVR light curves of BX Peg Virtual Observatory Resource

Authors
  1. Lee J.W.
  2. Kim S.-L.
  3. Lee C.-U.
  4. Youn J.-H.
  5. Published by
    CDS
Abstract

We present the results of new CCD photometry for the contact binary BX Peg, made during three successive months beginning on 2008 September. As do historical light curves, our observations display an O'Connell effect and the November data by themselves indicate clear evidence for very short-term brightness disturbance.

Keywords
  1. eclipsing-binary-stars
  2. ccd-photometry
  3. infrared-photometry
  4. visible-astronomy
  5. Wide-band photometry
Bibliographic source Bibcode
2009PASP..121.1366L
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/PASP/121/1366
IVOA Identifier IVOID
ivo://CDS.VizieR/J/PASP/121/1366

Access

Web browser access HTML
https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/PASP/121/1366
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/PASP/121/1366
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/PASP/121/1366
IVOA Table Access TAP
https://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).

History

2010-04-29T12:58:42Z
Resource record created
2010-04-29T12:58:42Z
Created
2017-07-06T06:26:08Z
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