UBV magnitude of NGC 884 B-type pulsators Virtual Observatory Resource

Authors

1. Krzesinski J.
2. Pigulski A.

Published by

CDS

Abstract

We present the results of the photometric CCD search for B-type pulsators in the central region of Chi Persei (NGC 884) open cluster. In addition to the two newly-discovered Beta Cephei stars we found 11 other variables in the observed field. The photometric data for them are given in the file 'bmag' and 'vmag' for B and V-filter data, respectively. In addition, we present the new UBV magnitudes for stars in the observed field. This is Table 4 of the paper, available only in electronic form.

Keywords

1. be-stars
2. visible-astronomy
3. Wide-band photometry
4. open-star-clusters

Bibliographic source Bibcode

1997A&A...325..987K

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/325/987

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/325/987

Document Object Identifer DOI

doi:10.26093/cds/vizier.33250987

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/325/987
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/325/987
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/325/987

IVOA Table Access TAP

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