6533b881fe1ef96bd12d8f59

RESEARCH PRODUCT

NW Ser and V1446 Aql uvby light curves

Gutierrez-soto J.Fabregat J.Suso J.Suarez J.c.Moya A.Garrido R.Hubert A.-m.Floquet M.Neiner C.Fremat Y.

subject

observational astronomyPhotometryMedium band photometryAstrophysics and AstronomyStellar AstronomyBe starsPhysicsNatural SciencesOptical astronomy

description

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.

https://dx.doi.org/10.26093/cds/vizier.34720565