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TOI-4600 b and c: Two Long-period Giant Planets Orbiting an Early K Dwarf

  • Authors: Ismael Mireles, Diana Dragomir, Hugh P. Osborn, Katharine Hesse, Karen A. Collins, Steven Villanueva, Allyson Bieryla, David R. Ciardi, Keivan G. Stassun, Mallory Harris, Jack J. Lissauer, Richard P. Schwarz, Gregor Srdoc, Khalid Barkaoui, Arno Riffeser, Kim K. McLeod, Joshua Pepper, Nolan Grieves, Vera Maria Passegger, Solène Ulmer-Moll, Joseph E. Rodriguez, Dax L. Feliz, Samuel Quinn, Andrew W. Boyle, Michael Fausnaugh, Michelle Kunimoto, Pamela Rowden, Andrew Vanderburg, Bill Wohler, Jon M. Jenkins, David W. Latham, George R. Ricker, Sara Seager, Joshua N. Winn

Ismael Mireles et al 2023 The Astrophysical Journal Letters 954 .

  • Provider: AAS Journals

Caption: Figure 5.

Top left: period–radius diagram of verified transiting planets orbiting stars with V < 13 (black) and V > 13 (gray), as of 2022 November (NASA Exoplanet Archive). Bottom left: equilibrium temperature diagram (assuming albedo a = 0) for the same sample. Right: the TOI-4600 system and other warm gas giant systems with multiple transiting planets. TOI-4600 c is the coldest and has the longest orbital period of any transiting planet in these systems.

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