The β Cephei star HD 167743

V. Antoci; G. Handler; R. Shobbrook; E. Romero-Colmenero; S. Barmania; R. Spann

doi:10.1088/1742-6596/118/1/012045

The β Cephei star HD 167743

V. Antoci^*, G. Handler, R. Shobbrook, E. Romero-Colmenero, S. Barmania, R. Spann

^*Corresponding author for this work

Research output: Contribution to journal › Article › peer-review

Abstract

The β Cephei star HD 167743 was observed from three different observatories in the years 2006 and 2007. The data sets were collected through the filters Johnson UBV and Strömgren uvy. First analyses show six independent and five combination frequencies. We present mode identifications, which are simplified by the rather high amplitudes of the star. No evidence for rotational splitting was found yet.

Original language	English
Article number	012045
Journal	Journal of Physics: Conference Series
Volume	118
Issue number	1
DOIs	https://doi.org/10.1088/1742-6596/118/1/012045
Publication status	Published - 1 Jul 2008

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AU - Handler, G.

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AU - Romero-Colmenero, E.

AU - Barmania, S.

AU - Spann, R.

PY - 2008/7/1

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The β Cephei star HD 167743

Abstract

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