Photometry of chemically peculiar stars Virtual Observatory Resource

Authors
  1. Adelman S.J.
  2. Published by
    CDS
Abstract

Differential Stromgren uvby photometric observations from the Four College Automated Photoelectric Telescope of four magnetic Chemically Peculiar stars are used to refine rotational periods and to define the shapes of the light curves. HR 1643 (P=2.73475d) shows large phase variability in all four magnitudes. Theta Aur (P=3.6188d) exhibits large amplitude variations with two components contributing to the minima. For 49 Cam (P=4.28679d), we probably are observing both polar regions and much of the surface. The values for HR 3724 (P=33.984d) confirm Wolff's result that the main variability is in v.

Keywords
  1. peculiar-variable-stars
  2. visible-astronomy
  3. medium-band-photometry
Bibliographic source Bibcode
1997PASP..109....9A
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/PASP/109/9
IVOA Identifier IVOID
ivo://CDS.VizieR/J/PASP/109/9

Access

Web browser access HTML
http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/PASP/109/9
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/PASP/109/9
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/PASP/109/9
IVOA Table Access TAP
http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).

History

1997-12-09T21:47:43Z
Resource record created
1997-12-09T20:47:50Z
Updated
1997-12-09T21:47:43Z
Created

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