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Formation of Giant Planets by Gas Disk Gravitational Instability on Wide Orbits around Protostars with Varied Masses. II. Quadrupled Spatial Resolution and Beta Cooling
Population of giant planets around B stars from the first part of the BEAST survey
P. Delorme, A. Chomez, V. Squicciarini, M. Janson, O. Flasseur, O. Schib, R. Gratton, A.-M. Lagrange, M. Langlois, L. Mayer, R. Helled, S. Reffert, F. Kiefer, B. Biller, G. Chauvin, C. Fontanive, Th. Henning, M. Kenworthy, G.-D. Marleau, D. Mesa, M. R. Meyer, C. Mordasini, S. C. Ringqvist, M. Samland, A. Vigan and G. Viswanath Astronomy & Astrophysics 692 A263 (2024) https://doi.org/10.1051/0004-6361/202451461
Planet Formation—Observational Constraints, Physical Processes, and Compositional Patterns