Linking Outer Disk Pebble Dynamics and Gaps to Inner Disk Water Enrichment

نویسندگان

چکیده

Millimeter continuum imaging of protoplanetary disks reveals the distribution solid particles and presence substructures (gaps rings) beyond 5-10 au, while infrared (IR) spectra provide access to abundances gaseous species at smaller disk radii. Building on recent observational findings an anti-correlation between inner water luminosity outer dust radius, we aim here investigating dynamics icy solids that drift from sublimate their ice inside snow line, enriching vapor is observed in IR. We use a volatile-inclusive evolution model explore range conditions (gap location, particle size, mass, alpha-viscosity) under which gaps efficiently block inward solids. find inner-disk enrichment highly sensitive location gap, yielding for each size radial "sweet spot" reduces minimum. For pebbles 1-10 mm carry most this sweet spot 7-15 suggesting may have key role reducing delivery not allow formation Earths super-Earths. This highlights importance observationally determining properties disks. Finally, argue abundance can be used as proxy estimating pebble efficiency mass-flux entering disk.

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ژورنال

عنوان ژورنال: The Astrophysical Journal

سال: 2021

ISSN: ['2041-8213', '2041-8205']

DOI: https://doi.org/10.3847/1538-4357/ac1e96