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Eleven New Transiting Brown Dwarfs and Very-low-mass Stars from TESS

  • Authors: Noah Vowell, Joseph E. Rodriguez, David W. Latham, Samuel N. Quinn, Jack Schulte, Jason D. Eastman, Allyson Bieryla, Khalid Barkaoui, David R. Ciardi, Karen A. Collins, Eric Girardin, Guillaume Hébrard, Elisabeth Heldridge, Marziye Jafariyazani, Brooke Kotten, Luigi Mancini, Felipe Murgas, Norio Narita, D. J. Radford, Howard M. Relles, Avi Shporer, Melinda Soares-Furtado, Ivan A. Strakhov, Carl Ziegler, Isabelle Boisse, César Briceño, Michael L. Calkins, Catherine A. Clark, Kevin I. Collins, Jerome de Leon, Gilbert A. Esquerdo, Sergio B. Fajardo-Acosta, Thierry Forveille, Akihiko Fukui, Cristilyn N. Watkins, Ruixuan He, Neda Heidari, Keith Horne, Jon M. Jenkins, Andrew W. Mann, Luca Naponiello, Enric Palle, Richard P. Schwarz, S. Seager, John Southworth, Gregor Srdoc, Jonathan J. Swift, Joshua N. Winn

Noah Vowell et al 2025 The Astronomical Journal 170 .

  • Provider: AAS Journals

Caption: Figure 14.

Left: eccentricity vs. mass for transiting BDs with a dotted line at the proposed B. Ma & J. Ge (2014) boundary between planet- and star-like BDs. Right: all transiting companions ranging from 7 to 150 MJ in eccentricity vs. mass ratio with a dashed line at the same 42 MJ location assuming a 1.0 M⊙ host star. As discussed in Section 4.1, the eccentricity dichotomy between low- and high-mass BDs does not hold up when plotted against mass ratio, suggesting that this feature may not represent the boundary between planet-like and star-like BDs.

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