{"public_id":"cl_eae6ef355155f771b3afe5a618533e5c","status":"active","superseded_by_public_id":null,"corpus_id":17528323,"text":"The outflows have axes perpendicular to the disks, exhibit proper motions up to about 42 km s-1, and are outlined by maser emission up to about 260 AU from the protostars.","confidence":0.96,"paper":{"corpus_id":17528323,"title":"Water Masers as Tracers of Protostellar Disks and Outflows in the Intermediate-Mass Star-forming Region NGC 2071","url":"https://sah.borca.ai/papers/17528323"},"contributors":[{"id":136,"public_id":"3c2apqe3ut","public_label":"Anonymous (3c2apqe3ut)","roles":["extraction"],"url":"https://sah.borca.ai/u/3c2apqe3ut"},{"id":2,"public_id":"4715169a40","public_label":"AK (4715169a40)","roles":["review"],"url":"https://sah.borca.ai/u/4715169a40"},{"id":1,"public_id":"12632b8b5f","public_label":"Anonymous (12632b8b5f)","roles":["review"],"url":"https://sah.borca.ai/u/12632b8b5f"}],"origin_summary":{"object_type":"claim","status":"active","confidence":0.96,"origin_kinds":["extraction","extraction_create"],"contribution_count":1,"contribution_task_types":["extraction"],"contribution_statuses":["applied"],"verifier_verdict_count":2,"verifier_classes":["system","user_agent"],"verifier_class_counts":{"system":1,"user_agent":1},"verdict_counts":{"approve":2,"reject":0},"verifier_state":"mixed","basis":["kg_settlement_results.decision_payload.legacy_bridge","kg_entity_origin_refs","kg_assertion_proposals","contributions","verifications","claim.status","claim.confidence"],"limits":["ledger provenance is aggregated; raw contribution and verifier audit rows are not expanded","entity matching uses settlement bridge refs and edge commands"]},"concepts":[{"public_id":"co_7d28de78473c3a6114c53275a604b828","name":"proper motions","description":"Measured motions of maser features used to infer dynamics in the disks and outflows.","types":["kinematic measurements"],"url":"https://sah.borca.ai/concepts/co_7d28de78473c3a6114c53275a604b828"},{"public_id":"co_f18de8328550be07ab3a69173988abf7","name":"protostars","description":"The young stellar objects associated with IRS 1 and IRS 3 from which the disk and outflow structures originate.","types":["stellar objects"],"url":"https://sah.borca.ai/concepts/co_f18de8328550be07ab3a69173988abf7"},{"public_id":"co_f942630da80031cce2c4a7277d08eca4","name":"outflows","description":"Protostellar flows in IRS 1 and IRS 3 outlined by maser emission extending away from the central sources.","types":["astronomical flows"],"url":"https://sah.borca.ai/concepts/co_f942630da80031cce2c4a7277d08eca4"}],"related_claims":[],"url":"https://sah.borca.ai/claims/cl_eae6ef355155f771b3afe5a618533e5c"}