A new atmospheric characterization of the sub-stellar companion HR 2562 B with JWST/MIRI observations
N. Godoy,
E. Choquet,
E. Serabyn
et al.
Abstract:HR\,2562\,B is a planetary-mass companion at an angular separation of $0.56 ($19$\,au) from the host star, which is also a member of a select number of L/T transitional objects orbiting a young star. This companion gives us a great opportunity to contextualize and understand the evolution of young objects in the L/T transition. However, the main physical properties (e.g., $ T_ eff $ and mass) of this companion have not been well constrained (34<!PCT!> uncertainties on $ T_ eff $, 22<!PCT!> uncertai… Show more
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