NW Ser and V1446 Aql uvby light curves

DOI

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.

Identifier
DOI http://doi.org/10.26093/cds/vizier.34720565
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/472/565
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/472/565
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/472/565
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/472/565
Provenance
Creator Gutierrez-Soto J.; Fabregat J.; Suso J.; Suarez J.C.; Moya A.; Garrido R.,Hubert A.-M.; Floquet M.; Neiner C.; Fremat Y.
Publisher CDS
Publication Year 2007
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy