Derivation of the orbit of a double star from observations made with an intensity interferometer

Published: 1 January 1971| Version 1 | DOI: 10.17632/p545cr4zg4.1
D. Herbison-Evans


Title of program: BIN DYN Catalogue Id: AACD_v1_0 Nature of problem The data from a stellar intensity interferometer consists of a set of observations of the correlation of the light from two optical reflectors with a given separation (the baseline). If the star is double the data can be used to find the orbit of the double star. This has been done for the star alpha Virginis. Versions of this program held in the CPC repository in Mendeley Data AACD_v1_0; BIN DYN; 10.1016/0010-4655(71)90016-6 This program has been imported from the CPC Program Library held at Queen's University Belfast (1969-2019)



Astronomy, Astrophysics, Computational Physics