Abstract
Orbits of 44 close and fast visual binaries are computed using the latest speckle observations; 23 orbits are determined for the first time, and the rest are revisions, some of those substantial. Six combined orbits use radial velocities. The median period is 15.6 years, and the shortest period is one year. Most stars are nearby late-type dwarfs. Dynamical parallaxes and estimates of the masses are derived from the orbital elements and the photometry of the components.
Cite
CITATION STYLE
Tokovinin, A. (2017). New Orbits Based on Speckle Interferometry at SOAR. II.*. The Astronomical Journal, 154(3), 110. https://doi.org/10.3847/1538-3881/aa8459
Register to see more suggestions
Mendeley helps you to discover research relevant for your work.