The orbit of LDS 720BC = CD -32 16135.
Abstract
Summary. A new orbit with period 675 yr is shown to represent satisfactorily all available observations of the binary star LDS 720BC. Mso the resulting dynamical parallax agrees well with the trigonometric, which was not the case for Mourao's 240-yr orbit found by his assuming quadrant reversal for the earliest measure made at Perth in 1913.
- Publication:
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Monthly Notices of the Royal Astronomical Society
- Pub Date:
- February 1978
- DOI:
- 10.1093/mnras/182.3.345
- Bibcode:
- 1978MNRAS.182..345W
- Keywords:
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- Orbits:Visual Binaries