Retrieving the C and O Abundances of HR 7672 AB: A Solar-type Primary Star with a Benchmark Brown Dwarf

Retrieving the C and O Abundances of HR 7672 AB: A Solar-type Primary Star with a Benchmark Brown Dwarf

A benchmark brown dwarf (BD) is a BD whose properties (e.g., mass and chemical composition) are precisely and independently measured. Benchmark BDs are valuable in testing theoretical evolutionary tracks, spectral synthesis, and atmospheric retrievals for substellar objects. Here, we report results...

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Main Authors: Baker, A. (Author), Bartos, R. (Author), Blake, G.A (Author), Bond, C.Z (Author), Calvin, B. (Author), Cetre, S. (Author), Delorme, J.-R (Author), Doppmann, G. (Author), Echeverri, D. (Author), Finnerty, L. (Author), Fitzgerald, M.P (Author), Jovanovic, N. (Author), Kent Wallace, J. (Author), Kolecki, J.R (Author), Liu, M.C (Author), Lopez, R. (Author), Mawet, D. (Author), Morris, E. (Author), Pai Asnodkar, A. (Author), Pezzato, J. (Author), Ragland, S. (Author), Roy, A. (Author), Ruane, G. (Author), Ruffio, J.-B (Author), Sappey, B. (Author), Schofield, T. (Author), Skemer, A. (Author), Venenciano, T. (Author), Wallack, N.L (Author), Wang, J. (Author), Wang, J.J (Author), Wizinowich, P. (Author), Xuan, J.W (Author)
Format: Article
Language:English
Published: American Astronomical Society 2022
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