ODISEA: Disk dust mass distributions
收藏B2FIND2026-03-19 收录
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https://b2find.eudat.eu/dataset/a003f00a-c8dc-516a-ac73-f1d77af26b84
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As protostars evolve from optically faint/infrared-bright (Class I) sources to optically bright/infrared-faint (Class II) the solid material in their surrounding disks...
