The modeling of the physical and dynamical properties of spectroscopic binaries with an orbitdoctoral dissertation

Abstract

The innovative idea of this study is to establish a mathematical algorithm that permits us to determine the most probable model that explain the physical properties for each spectroscopic binary (those that they are not resolved with optic techniques)with an orbit and parallax and to extend the orbit to three dimensions. Once this is achieved, it will possible to answer the question regarding what telescope is necessary to resolve each of them, and to answer which of these binary sytems can be hosts of exoplanets with stable orbits