Intriguing, Low-amplitude Periodicity in the Radial Velocities of delta Sagittarrii

Astronomy and Astrophysics – Astronomy

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Scientific paper

We present the initial results of the analysis of the precise radial velocities of the relatively little-studied star delta Sagittarii, K2.5 IIIa, HR 6859. The data were obtained at the Canada-France-Hawaii Telescope using the hydrogen fluoride absorption cell technique. The periodogram shows significant peaks at 2.8 days (K=104 m s(-1) ), 63 days (K=85 m s(-1) ), and 295 days (K=72 m s(-1) ). Because of our limited data the true period cannot be distinguished from these possibilities due to aliasing. This giant is an interesting example of a star having a radial velocity periodicity which may be attributed to intrinsic variability, rotational modulation, or the presence of a low M_2 sin i companion (see A. Walker et al., this conference). More observations are urgently required to determine the true period and to discover the underlying origin for this star's radial velocity variability.

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