[en] The lowest-mass stars, brown dwarfs and giant exoplanets span a minimum in the mass-radius relationship that probes the fundamental physics of extreme states of matter, magnetism, and fusion. This White Paper outlines scientific opportunities and the necessary resources for modeling and measuring the mass- radius relationship in this regime. <P />
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Burgasser, Adam; UC San Diego
Baraffe, Isabelle; University of Exeter
Browning, Matthew; University of Exeter
Burrows, Adam; Princeton University
Chabrier, Gilles; University of Exeter
Creech-Eakman, Michelle; New Mexico Tech
Demory, Brice; University of Bern
Dieterich, Sergio; Carnegie DTM
Faherty, Jacqueline; American Museum of Natural History
Huber, Daniel; University of Hawaii
Lodieu, Nicolas; Instituto de Astrofisica de Canarias
Plavchan, Peter; George Mason University
Rich, R. Michael; UC Los Angeles
Saumon, Didier; Los Alamos National Laboratory
Stassun, Keivan; Vanderbilt University
Triaud, Amaury; University of Birmingham
van Belle, Gerard; Lowell Observatory
Van Grootel, Valérie ; Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique stellaire théorique et astérosismologie
Vos, Johanna M.; American Museum of Natural History
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