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Table · dataset · 1971

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

Listed in Teesside University Research Data Repository

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).

Description

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)

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Where it is published

Catalogue records · 1

Topics

From keywords
Astronomy & Astrophysics · Earth & Environmental Science · Physics
Provenance · 1 source records, 8 field assertions
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Teesside University Research Data Repositoryoai:data.mendeley.com/p545cr4zg4.115 h agoJSON v1
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concepts[field].local:field:astronomymapping · researchdata tees ac ukconnector:researchdata_tees_ac_uk@1.0.0
concepts[field].local:field:earth-environmentalmapping · researchdata tees ac ukconnector:researchdata_tees_ac_uk@1.0.0
concepts[field].local:field:physicsmapping · researchdata tees ac ukconnector:researchdata_tees_ac_uk@1.0.0
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