Spectroscopic study measures new orbital parameters for Trapezium components A, B, and D, confirms a tertiary in B, and finds Component F likely unrelated due to discrepant radial velocity.
J., Lloyd C., 2000, The Observatory , 120 , 141
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Multiplicity of the Orion Trapezium stars
Spectroscopic study measures new orbital parameters for Trapezium components A, B, and D, confirms a tertiary in B, and finds Component F likely unrelated due to discrepant radial velocity.