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Turbulence Inhibits Planetesimal Formation in Class 0/I Disks Subject to Infall
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FAUST
G. Sabatini, E. Bianchi, C. J. Chandler, L. Cacciapuoti, L. Podio, M. J. Maureira, C. Codella, C. Ceccarelli, N. Sakai, L. Testi, C. Toci, B. Svoboda, T. Sakai, M. Bouvier, P. Caselli, N. Cuello, M. De Simone, I. Jímenez-Serra, D. Johnstone, L. Loinard, Z. E. Zhang and S. Yamamoto Astronomy & Astrophysics 698 L16 (2025) https://doi.org/10.1051/0004-6361/202554750
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Surface accretion as a dust retention mechanism in protoplanetary disks. I. Formulation and proof-of-concept simulations
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Grain Size in the Class I Protostellar System TMC-1A Constrained with ALMA and Very Large Array Observations
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There is no disk mass budget problem of planet formation
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Ken Rice, Hans Baehr, Alison K Young, Richard Booth, Sahl Rowther, Farzana Meru, Cassandra Hall and Adam Koval Monthly Notices of the Royal Astronomical Society 539(4) 3421 (2025) https://doi.org/10.1093/mnras/staf714
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