The β Cephei star HD 167743

Details The β Cephei star HD 167743 The β Cephei star HD 167743

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008jphcs.118a2045a&link_type=abstract

Journal of Physics: Conference Series, Volume 118, Issue 1, pp. 012045 (2008).

Physics

Scientific paper

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.

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