Concerning the planetary system of Barnard's star |
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Authors: | David C. Black Graham C.J. Suffolk |
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Affiliation: | Theoretical Studies Branch, Space Science Division, Ames Research Center, Moffett Field, California 94035 USA |
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Abstract: | The data pertaining to the proper motion of Barnard's Star are reanalyzed, It is shown that at least two dark compan ions are required to explain the observations. It is found that the orbits of the two companions (B1 and B2) are not coplanar, but have relative inclination ?50°. |
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