NW Ser and V1446 Aql uvby light curves Virtual Observatory Resource

Authors

1. Gutierrez-Soto J.
2. Fabregat J.
3. Suso J.
4. Suarez J.C.
5. Moya A.
6. Garrido R.,Hubert A.-M.
7. Floquet M.
8. Neiner C.
9. Fremat Y.

Published by

CDS

Abstract

We present accurate photometric time series of two Be stars: NW Ser and V1446 Aql. Both stars were observed at the Observatorio de Sierra Nevada (Granada) in July 2003 with an automatic four-channel Stroemgren photometer. We also present a preliminary theoretical study showing that the periodic variations exhibited by these stars can be due to pulsation.

Keywords

1. be-stars
2. visible-astronomy
3. medium-band-photometry

Bibliographic source Bibcode

2007A&A...472..565G

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/472/565

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/472/565

Document Object Identifer DOI

doi:10.26093/cds/vizier.34720565

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/472/565
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/472/565
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/472/565

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