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A Long Period Stellar-mass Black Hole Binary in ω Centauri

  • Authors: Matthew Whitaker, Evan Kerr, Anil Seth, Maximilian Häberle, Jay Strader, Jay Anderson, Andrea Bellini, Callie Clontz, Zack Freeman, Massimo Griggio, Sebastian Kamann, Mattia Libralato, Nadine Neumayer, Elena González Prieto, Carl L. Rodriguez, Sara Saracino, Peter Smith, Glenn van de Ven, Zixian Wang

Matthew Whitaker et al 2026 The Astrophysical Journal Letters 1006 .

  • Provider: AAS Journals

Caption: Figure 4.

Best-fit orbital model. Left: our median model (purple line) shown compared to the data after subtracting out the derived proper motion. The marker shape and color correspond to the instrument used for measurement, and the gray points represent 3σ outliers from the median fit. Right: our median orbital model plotted with the on-sky data in the proper-motion subtracted frame colored by observation date; the orbit is shown as a dashed line outside our observation window.

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