Figure 8 from Forty-four New and Known M-dwarf Multiples in the SDSS-III/APOGEE M-dwarf Ancillary Science Sample

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Forty-four New and Known M-dwarf Multiples in the SDSS-III/APOGEE M-dwarf Ancillary Science Sample

Authors: Jacob Skinner, Kevin R. Covey, Chad F. Bender, Noah Rivera, Nathan De Lee, Diogo Souto, Drew Chojnowski, Nicholas Troup, Carles Badenes, Dmitry Bizyaev, Cullen H. Blake, Adam Burgasser, Caleb Cañas, Joleen Carlberg, Yilen Gómez Maqueo Chew, Rohit Deshpande, Scott W. Fleming, J. G. Fernández-Trincado, D. A. García-Hernández, Fred Hearty, Marina Kounkel, Penélope Longa-Peñe, Suvrath Mahadevan, Steven R. Majewski, Dante Minniti, David Nidever, Audrey Oravetz, Kaike Pan, Keivan Stassun, Ryan Terrien, and Olga Zamora

2018 The Astronomical Journal 156 45.

Provider: AAS Journals

Caption: Figure 8.

Figures for 2M06115599+3325505, with ﹩{ \mathcal L }=56 \% ﹩ at P = 2.63 days. (Top) Lomb–Scargle periodogram power as a function of period (black) and the histogram of MCMC samples obtained during the period search (red). (Bottom left) Corner plot of the posterior probability distribution given by the random walk. (Bottom right) RV plot of this system. The solid blue curve is the primary component velocity, and the red dashed curve is the secondary component velocity. Primary component velocities are marked as squares, and secondary velocities are marked as circles.

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