Light Curves of RS Pup Virtual Observatory Resource

Authors
  1. Berdnikov L.N.
  2. Henden A.A.
  3. Turner D.G.
  4. Pastukhova E.N.
  5. Published by
    CDS
Abstract

Based on photographic plates from the Harvard College Observatory, we have made 1492 magnitude estimates for the long-period classical Cepheid RS Pup (P=41.4d). Together with the observations taken from the literature, our data have allowed us to construct an O-C diagram spanning a time interval of 135-years.

Keywords
  1. variable-stars
  2. photometry
Bibliographic source Bibcode
2009PAZh...35..451B
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/PAZh/35/451
IVOA Identifier IVOID
ivo://CDS.VizieR/J/PAZh/35/451

Access

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

History

2009-09-16T22:32:16Z
Resource record created
2009-09-16T22:32:16Z
Created
2017-06-26T11:50:00Z
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