Figure 12 from Diffraction-limited Visible Light Images of Orion Trapezium Cluster with the Magellan Adaptive Secondary Adaptive Optics System (MagAO)

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Diffraction-limited Visible Light Images of Orion Trapezium Cluster with the Magellan Adaptive Secondary Adaptive Optics System (MagAO)

Authors: L. M. Close, J. R. Males, K. Morzinski, D. Kopon, K. Follette, T. J. Rodigas, P. Hinz, Y-L. Wu, A. Puglisi, S. Esposito, A. Riccardi, E. Pinna, M. Xompero, R. Briguglio, A Uomoto, and T. Hare

Close et al. 2013 The Astrophysical Journal 774 94.

Provider: AAS Journals

Caption: Figure 12.

Separation between the θ ¹ Ori B ₂ and B ₃ components. Note the surprising lack of any significant relative motion (−0.04 ± 0.14 mas yr ⁻¹). The rms scatter from a constant value is only 0.14 mas yr ⁻¹. There appears to be very little change in the separation of the B ₂ B ₃ system. The epochs of the data are the same as in Figure 10.

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