ON SHOCKS DRIVEN BY HIGH-MASS PLANETS IN RADIATIVELY INEFFICIENT DISKS. II. THREE-DIMENSIONAL GLOBAL DISK SIMULATIONS
Wladimir Lyra(Lowell Observatory), Mario Flock(Jet Propulsion Laboratory), Satoshi Okuzumi(Tokyo Institute of Technology), Alexander J. W. Richert(Pennsylvania State University), Mordecai‐Mark Mac Low(American Museum of Natural History), Aaron C. Boley(University of British Columbia), N. Turner(Andrews University)
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