| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1782101 | Planetary and Space Science | 2008 | 5 Pages |
Abstract
The estimations of the masses for some binaries are discussed. Also we justify the necessity of precise parallaxes and relative radial velocities of stars, which could be measured by space telescopes such as the GAIA as the additional parameters for determination of orbits of binaries.
Keywords
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Geophysics
Authors
N.A. Shakht, A.A. Kisselev,