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Sierra Grant
sierragrant.bsky.social
did:plc:o7m7dpplpha4had22kkzpsjo
The JWST-MIRI spectrum is extremely line-rich with a forest of H2O lines. DF Tau A and B are not resolved with JWST, therefore the spectrum must be taken as the sum of both disks. We suggest that DF Tau B has a small cavity (~1 au) and that most of the emission is coming from A.
2024-07-15T10:11:14.648Z