Disc population synthesis: Decrease in the solid mass reservoir through pebble drift

نویسندگان

چکیده

Surveys of star-forming regions reveal that the dust mass protoplanetary discs decreases by several orders magnitude on a timescale few million years. This decrease in budget solids is likely due to gas-drag-induced radial drift mm-sized solids, called pebbles. However, quantifying evolution this component young stellar clusters difficult inherent large spread masses and formation times. Therefore, we aim model collective cluster investigate effectiveness clearing particles. We use disc numerically solves for formation, viscous photoevaporative gas component, while also including particles limited size fragmentation. find are born with between 50 Earth 1000 masses, stars with, respectively, 0.1 solar 1 masses. The majority initial reservoir typically lost through before photoevaporation opens gap models both without strong X-ray-driven loss rates. conclude time locked fragmentation-limited pebbles consistent ages inferred from nearby when assuming rates corresponding mean lifetimes 3 Myr 8 Myr.

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ژورنال

عنوان ژورنال: Astronomy and Astrophysics

سال: 2023

ISSN: ['0004-6361', '1432-0746']

DOI: https://doi.org/10.1051/0004-6361/202245252