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The pulsating lambda Bootis star HD 105759

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Abstract

We present spectroscopic and multisite time series photometric observations of the star HD 105759 which confirm that this is a new pulsating lambda Bootis star. Our spectroscopy indicates an overall metallicity of [Z]=log Z-log Z_solar=-1 and that T_eff=8000+/-300 K and logg=4.0+/-0.2. The photometric data reveal that this star pulsates with at least five frequencies: 8.62, 12.69, 20.15, 21.27 and 23.66 d^-1. These frequencies do not all match those found in an earlier single-site study, indicating that the pulsation spectrum changes with time.


Publication:

Monthly Notices of the Royal Astronomical Society

Pub Date:
December 1998
DOI:

10.1046/j.1365-8711.1998.02070.x

Bibcode:
1998MNRAS.301.1099M
Keywords:
  • STARS: CHEMICALLY PECULIAR;
  • STARS: INDIVIDUAL: HD 105759;
  • STARS: OSCILLATIONS;
  • STARS: VARIABLES: OTHER