Image Details
Caption: Figure 13.
Radius vs. mass for all transiting companions from 7 to 150 MJ. The black dashed lines depict the canonical 13 and 80 MJ BD boundaries. The solid purple line at 42 MJ shows the proposed B. Ma & J. Ge (2014) boundary between planet- and star-like BDs. Note, systems where the primary object is a white dwarf or brown dwarf are not shown. References: B. A. Henderson et al. (2024b) and references therein as well as G. Á. Bakos et al. (2010), L. A. Buchhave et al. (2011), B. Tingley et al. (2011), H. Parviainen et al. (2014), A. S. Bonomo et al. (2015), L. J. Esteves et al. (2015), K. G. Stassun et al. (2017), J. Bento et al. (2018), C. I. Cañas et al. (2018), B. F. Cooke et al. (2020), P. Cortés-Zuleta et al. (2020), K. El-Badry et al. (2023), M. Lambert et al. (2023), S. P. Schmidt et al. (2023), P. A. Dalba et al. (2024), Y. T. Davis et al. (2024), J. Eberhardt et al. (2023), B. A. Henderson et al. (2024a), M. I. Swayne et al. (2024), and J.-Q. Wang et al. (2024).
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© 2025. The Author(s). Published by the American Astronomical Society.
