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The ESO SupJup Survey. III. Confirmation of 13CO in YSES 1 b and Atmospheric Detection of YSES 1 c with CRIRES+

  • Authors: Yapeng Zhang, Darío González Picos, Sam de Regt, Ignas A. G. Snellen, Siddharth Gandhi, Christian Ginski, Aurora Y. Kesseli, Rico Landman, Paul Mollière, Evert Nasedkin, Alejandro Sánchez-López, Tomas Stolker, Julie Inglis, Heather A. Knutson, Dimitri Mawet, Nicole Wallack, Jerry W. Xuan

Yapeng Zhang et al 2024 The Astronomical Journal 168 .

  • Provider: AAS Journals

Caption: Figure 10.

Rotation velocities (assuming isotropic inclination distribution) as a fraction of break-up velocities for super-Jovian companions. Our measurements of YSES 1 b and c are denoted with red diamonds. The measurements of other companions are adopted from the literature, including M. L. Bryan et al. (2020b), J. J. Wang et al. (2021), and. W. Xuan et al. (2024a). The data are color-coded by the companion masses. The blue data points show the spin of Jupiter and Saturn in the solar system.

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