{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:5YCTH3JY2U7J2DLP57N5VBDDWC","short_pith_number":"pith:5YCTH3JY","schema_version":"1.0","canonical_sha256":"ee0533ed38d53e9d0d6fefdbda8463b0a3b1778b724307514eccad8e9a120672","source":{"kind":"arxiv","id":"2410.18033","version":1},"attestation_state":"computed","paper":{"title":"JWST/NIRSpec Reveals the Nested Morphology of Disk Winds from Young Stars","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.EP","authors_text":"Bennett N. Skinner, Colette Salyk, Dmitry Semenov, Fabien Louvet, Gaspard Duchene, Ilaria Pascucci, James Muzerolle Page, Joan Najita, Kamber Schwarz, Marion Villenave, Maxime Ruaud, Naman S. Bajaj, Sean D. Brittain, Sebastiaan Krijt, Suzan Edwards, Sylvie Cabrit, Tracy L. Beck, Uma Gorti","submitted_at":"2024-10-23T17:03:41Z","abstract_excerpt":"Radially extended disk winds could be the key to unlocking how protoplanetary disks accrete and how planets form and migrate. A distinctive characteristic is their nested morphology of velocity and chemistry. Here we report JWST/NIRSpec spectro-imaging of four young stars with edge-on disks in the Taurus star-forming region that demonstrate the ubiquity of this structure. In each source, a fast collimated jet traced by [Fe II] is nested inside a hollow cavity within wider lower-velocity H2 and, in one case, also CO ro-vibrational (v=1-0) emission. Furthermore, in one of our sources, ALMA CO(2-"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"2410.18033","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.EP","submitted_at":"2024-10-23T17:03:41Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"2478be45bebee0688b87fef6c7a9a7d9853c525cefa481a311c4a8e2a3be89b0","abstract_canon_sha256":"917d95d8cd8fee535e932b929ab660f9d8c24da8fef67ddbb1003793f8c444e9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:24:48.375452Z","signature_b64":"G2q4rMBRJyFiWpPTj6/ldcs0BH1ygmn67lu84BqEEd3XkU7BKuJdgNR2yOZBxwIjx3J9Z47qwAFpp5h4QEz/AQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ee0533ed38d53e9d0d6fefdbda8463b0a3b1778b724307514eccad8e9a120672","last_reissued_at":"2026-07-05T09:24:48.374954Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:24:48.374954Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"JWST/NIRSpec Reveals the Nested Morphology of Disk Winds from Young Stars","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.EP","authors_text":"Bennett N. Skinner, Colette Salyk, Dmitry Semenov, Fabien Louvet, Gaspard Duchene, Ilaria Pascucci, James Muzerolle Page, Joan Najita, Kamber Schwarz, Marion Villenave, Maxime Ruaud, Naman S. Bajaj, Sean D. Brittain, Sebastiaan Krijt, Suzan Edwards, Sylvie Cabrit, Tracy L. Beck, Uma Gorti","submitted_at":"2024-10-23T17:03:41Z","abstract_excerpt":"Radially extended disk winds could be the key to unlocking how protoplanetary disks accrete and how planets form and migrate. A distinctive characteristic is their nested morphology of velocity and chemistry. Here we report JWST/NIRSpec spectro-imaging of four young stars with edge-on disks in the Taurus star-forming region that demonstrate the ubiquity of this structure. In each source, a fast collimated jet traced by [Fe II] is nested inside a hollow cavity within wider lower-velocity H2 and, in one case, also CO ro-vibrational (v=1-0) emission. Furthermore, in one of our sources, ALMA CO(2-"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2410.18033","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2410.18033/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"2410.18033","created_at":"2026-07-05T09:24:48.375016+00:00"},{"alias_kind":"arxiv_version","alias_value":"2410.18033v1","created_at":"2026-07-05T09:24:48.375016+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2410.18033","created_at":"2026-07-05T09:24:48.375016+00:00"},{"alias_kind":"pith_short_12","alias_value":"5YCTH3JY2U7J","created_at":"2026-07-05T09:24:48.375016+00:00"},{"alias_kind":"pith_short_16","alias_value":"5YCTH3JY2U7J2DLP","created_at":"2026-07-05T09:24:48.375016+00:00"},{"alias_kind":"pith_short_8","alias_value":"5YCTH3JY","created_at":"2026-07-05T09:24:48.375016+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.07571","citing_title":"Ionized gas emission in protoplanetary disks with the SKAO","ref_index":69,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/5YCTH3JY2U7J2DLP57N5VBDDWC","json":"https://pith.science/pith/5YCTH3JY2U7J2DLP57N5VBDDWC.json","graph_json":"https://pith.science/api/pith-number/5YCTH3JY2U7J2DLP57N5VBDDWC/graph.json","events_json":"https://pith.science/api/pith-number/5YCTH3JY2U7J2DLP57N5VBDDWC/events.json","paper":"https://pith.science/paper/5YCTH3JY"},"agent_actions":{"view_html":"https://pith.science/pith/5YCTH3JY2U7J2DLP57N5VBDDWC","download_json":"https://pith.science/pith/5YCTH3JY2U7J2DLP57N5VBDDWC.json","view_paper":"https://pith.science/paper/5YCTH3JY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2410.18033&json=true","fetch_graph":"https://pith.science/api/pith-number/5YCTH3JY2U7J2DLP57N5VBDDWC/graph.json","fetch_events":"https://pith.science/api/pith-number/5YCTH3JY2U7J2DLP57N5VBDDWC/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5YCTH3JY2U7J2DLP57N5VBDDWC/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5YCTH3JY2U7J2DLP57N5VBDDWC/action/storage_attestation","attest_author":"https://pith.science/pith/5YCTH3JY2U7J2DLP57N5VBDDWC/action/author_attestation","sign_citation":"https://pith.science/pith/5YCTH3JY2U7J2DLP57N5VBDDWC/action/citation_signature","submit_replication":"https://pith.science/pith/5YCTH3JY2U7J2DLP57N5VBDDWC/action/replication_record"}},"created_at":"2026-07-05T09:24:48.375016+00:00","updated_at":"2026-07-05T09:24:48.375016+00:00"}