UBV Photometry of phi Per Virtual Observatory Resource

Authors

1. Bozic H.
2. Harmanec P.
3. Horn J.
4. Koubsky P.
5. Scholz G.
6. McDavid D.,Hubert A.-M.
7. Hubert H.

Published by

CDS

Abstract

A detailed analysis of a very rich collection of spectroscopic and photometric observations of the bright Be star {phi} Per (HR 496, or HD 10516, 2000 position: 01 43 39.4 +50 41 20) is presented. Earlier reports that {phi} Per is a double-lined spectroscopic binary consisting of two emission-line objects are confirmed.

Keywords

1. visible-astronomy
2. Wide-band photometry
3. variable-stars

Bibliographic source Bibcode

1995A&A...304..235B

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/304/235

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/304/235

Document Object Identifer DOI

doi:10.26093/cds/vizier.33040235

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/304/235
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/304/235
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/304/235

IVOA Table Access TAP

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