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What is Planetesimal Formation in Pressure Bumps about?

This study investigates planetesimal formation in protoplanetary disks due to pressure bumps caused by the infall of interstellar material. A numerical model is developed to analyze the conditions that favor this process, finding that infall-induced pressure bumps can effectively trap dust and enhance its growth, leading to planetesimal formation. The research concludes that such pressure bumps are advantageous for planetesimal formation without requiring preexisting massive planets.

Author

yoled68082

Language

EN