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

Ji Wang(University of Florida), Jerry W. Xuan(California Institute of Technology), Nemanja Jovanović(California Institute of Technology), Jacques-Robert Delorme(California Institute of Technology), Tobias Schofield(National Aquarium), Nicole L. Wallack(California Institute of Technology), Anusha Pai Asnodkar(The Ohio State University), Jacklyn Pezzato(California Institute of Technology), Arpita Roy(California Institute of Technology), Luke Finnerty, Evan Morris(University of California, Santa Cruz), Randall Bartos(Jet Propulsion Laboratory), J. Kent Wallace(California Institute of Technology), Ashley Baker(California Institute of Technology), Jean-Baptiste Ruffio(California Institute of Technology), Sam Ragland, Dimitri Mawet(European Southern Observatory), Sylvain Cetre(W.M. Keck Observatory), Daniel Echeverri(California Institute of Technology), Peter Wizinowich(Durham University), Garreth Ruane, Geoffrey A. Blake(California Institute of Technology), Ronald López(University of California, Los Angeles), Ben Sappey(University of California San Diego), Jared Kolecki(The Ohio State University), Benjamin Calvin(California Institute of Technology), Greg Doppmann(Kitt Peak National Observatory), Michael P. Fitzgerald(Lawrence Livermore National Laboratory), Michael C. Liu(University of Hawaii System), Jason Wang(Northwestern University), Andrew Skemer(University of Arizona), Charlotte Z. Bond(Royal Observatory), Taylor Venenciano(Pomona College)
The Astronomical Journal
March 25, 2022
Cited by 43


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