The Orbit of the Binary Star Delta Scorpii

Astronomy and Astrophysics – Astrophysics

Scientific paper

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(LaTex 8 pages. Send email to 'tbedding@eso.org' for 4 postscript figures). To appear in the Astronomical Journal, August, 199

Scientific paper

10.1086/116684

Although delta Scorpii is a bright and well-studied star, the details of its multiplicity have remained unclear. Here we present the first diffraction-limited image of this 0.12 arcsec binary star, made using optical interferometry, and resolve the confusion that has existed in the literature over its multiplicity. Examining published speckle measurements, together with the present result, reveals a periodicity of 10.5 yr and allows calculation of the orbital parameters. The orbit has a high eccentricity (e=0.82) and large inclination (i=70 degrees), making it a favourable target for radial velocity measurements during the next periastron (in 2000).

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