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Calculating the Apparent Orbit of a Double Star

© 2005. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Richard L. Branham, Jr. 2005 ApJ 622 613 DOI 10.1086/427870

0004-637X/622/1/613

Abstract

A method is given, based on the recently developed mathematical discipline of semidefinite programming, to calculate the apparent orbit of a double star. The method allows for outliers in the data and calculates mean errors for the derived quantities. An orbit, based on 128 observations, for the double star 24 Aquarii is calculated.

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10.1086/427870