Figure 9 from SOAR TESS Survey. I. Sculpting of TESS Planetary Systems by Stellar Companions

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SOAR TESS Survey. I. Sculpting of TESS Planetary Systems by Stellar Companions

Authors: Carl Ziegler, Andrei Tokovinin, César Briceño, James Mang, Nicholas Law, and Andrew W. Mann

2020 The Astronomical Journal 159 19.

Provider: AAS Journals

Caption: Figure 9.

Similar to Figure 5 for TESS M dwarf planet candidate hosts, using the field binary statistics of Winters et al. (2019). As with the solar-type stars, the M dwarf planet candidate hosts have a deficit of close binaries at separations less than 100 au and a surplus of wide binaries separated by more than 100 au.

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