Image Details
Caption: Figure 13.
Comparison of the stellar mass and estimated companion mass (left) and of the stellar mass and projected companion separation (right). For the companion masses, we denote the boundary between brown dwarfs and stars (hydrogen burning limit: blue) and denote the boundary between planets and brown dwarfs (deuterium burning limit: orange).
© 2022. The Author(s). Published by the American Astronomical Society.