Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995aas...18710213w&link_type=abstract
American Astronomical Society, 187th AAS Meeting, #102.13; Bulletin of the American Astronomical Society, Vol. 27, p.1430
Astronomy and Astrophysics
Astronomy
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.
Irwin Alan W.
Larson Ana M.
Walker Andrew R.
Walker Gordon A. H.
Yang Stephenson L. S.
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