Detection of a star escaping from the Orion Trapezium

  title={Detection of a star escaping from the Orion Trapezium},
  author={Eh. A. Vitrichenko and Holger Lehmann and Valentina Klochkova and Larisa Vladimirovna Bychkova and V. D. Bychkov},
During studies of spectra of the star Θ1 Ori C with high photometric and spectral resolution we have discovered a system of spectral lines indicating a large negative radial velocity (RV). We designate this star as Θ1 Ori C3. 
1 Citations
The companion C1 in the Θ1 Ori C system
The star Θ1 Ori C1, which is the nearest companion of the principal star Θ1 Ori C, is studied using extensive spectral data. Two radial velocity curves are constructed and solved. One of these


Low-Mass Runaway Stars from the Orion Trapezium Cluster
In the course of a search for common proper-motion binaries in the Jones & Walker (JW) catalog of proper motions in the Orion Nebula Cluster, we came across several faint stars with proper motions
Book-Review - the Orion Complex - a Case Study of Interstellar Matter
1: Large Scale View of the Orion Region.- 1.1. General Morphology of Barnard's Loop and the Neighbouring Region.- 1.2. Nature of Barnard's Loop and the Associated Filamentary Structure.- 1.3. Origin