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Stellar and Orbital Characterization of Three Low Mass M Dwarf Binary Stars with Dynamical Spectroscopy from the Habitable Zone Planet Finder

  • Authors: Suhani Surana, Chad F. Bender, Caleb I. Cañas, Daniel M. Krolikowski, William D. Cochran, Mark Everett, Arvind F. Gupta, Shubham Kanodia, Suvrath Mahadevan, Andrew Monson, Joe P. Ninan, Leonardo A. Paredes, Paul Robertson, Arpita Roy, Christian Schwab, Gudmundur Stefansson

Suhani Surana et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 2.

Robo-AO contrast curves for NLTT 43564 obtained with the Robo-AO laser Adaptive Optics system. The curves show the 5σ detection limits (Δm) as a function of angular separation. The inset of 1″ × 1″ shows the reconstructed speckle image at 832 nm. No nearby companions are detected within 1﹩\mathop{.}\limits^{\unicode{x02033}}﹩6 angular separation of the target.

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