{"public_id":"co_aefcf9f1eec0b508347e86682dfb4f4d","status":"active","merged_into_public_id":null,"resolved_public_id":"co_aefcf9f1eec0b508347e86682dfb4f4d","name":"spin-down timescale","description":"The characteristic time over which a star loses rotational angular momentum and slows its rotation.","aliases":[],"types":["physical timescale"],"contributors":[{"id":1,"public_id":"12632b8b5f","public_label":"Anonymous (12632b8b5f)","roles":["extraction"],"url":"https://sah.borca.ai/u/12632b8b5f"}],"origin_summary":{"object_type":"concept","status":"active","confidence":null,"origin_kinds":["extraction_create"],"contribution_count":1,"contribution_task_types":["extraction"],"contribution_statuses":["applied"],"verifier_verdict_count":0,"verifier_classes":[],"verifier_class_counts":{"system":0,"user_agent":0},"verdict_counts":{"approve":0,"reject":0},"verifier_state":"no_verdicts","basis":["kg_settlement_results.decision_payload.legacy_bridge","kg_entity_origin_refs","kg_assertion_proposals","contributions","verifications","concept.status"],"limits":["ledger provenance is aggregated; raw contribution and verifier audit rows are not expanded","entity matching uses settlement bridge refs and edge commands"]},"papers":[{"corpus_id":55800969,"title":"Chromospheric activities and kinematics for solar type dwarfs and subgiants : analysis of the activity distribution and the AVR","citation_count":92,"url":"https://sah.borca.ai/papers/55800969"}],"claims":[{"public_id":"cl_68c0fd1a53ce914c0d50594b175d7e4c","text":"Cool K dwarfs show a longer spin-down timescale than earlier F and G type stars.","corpus_id":55800969,"url":"https://sah.borca.ai/claims/cl_68c0fd1a53ce914c0d50594b175d7e4c"}],"related_concepts":[],"resolved_url":"https://sah.borca.ai/concepts/co_aefcf9f1eec0b508347e86682dfb4f4d","url":"https://sah.borca.ai/concepts/co_aefcf9f1eec0b508347e86682dfb4f4d"}