{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:BGPSWLGAHAEWEQYS4TLS2AZO7D","short_pith_number":"pith:BGPSWLGA","schema_version":"1.0","canonical_sha256":"099f2b2cc03809624312e4d72d032ef8fa0b4fa65fd11d873b6eba328cb97344","source":{"kind":"arxiv","id":"1611.06382","version":1},"attestation_state":"computed","paper":{"title":"Investigating the rotational evolution of very low-mass stars and brown dwarfs in young clusters using Monte Carlo simulations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"J. Bouvier, M. J. Vasconcelos","submitted_at":"2016-11-19T15:27:37Z","abstract_excerpt":"Context. Very low-mass (VLM) stars and brown dwarfs (BDs) present a different rotational behaviour from their solar mass counter-parts. Aims. We investigate the rotational evolution of young VLM stars and BDs using Monte Carlo simulations under the hypothesis of disk locking and stellar angular momentum conservation. Methods. We built a set of objects with masses ranging from 0.01 Mo to 0.4 Mo and considered models with single- and double- peaked initial period distributions with and without disk locking. An object is considered to be diskless when its mass accretion rate is below a given thre"},"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":"1611.06382","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2016-11-19T15:27:37Z","cross_cats_sorted":[],"title_canon_sha256":"7820d387111afcefac3dc7d5eaf7002e3fed0dad3f9f8ebed4478687d27283dd","abstract_canon_sha256":"68bb94a3e54a2fd978cfa6ea7ae6197c459d57a96d06e05a5c5b79f804636f18"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:46:38.943350Z","signature_b64":"n2lhgWO1wuwWbVj3UmjxYJnKoP2X0lWvUGkqDtKA/b9tCo/D/Cec6MdRWT6VIo2TlT1CQwM2Hq8SlaVvHXHhDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"099f2b2cc03809624312e4d72d032ef8fa0b4fa65fd11d873b6eba328cb97344","last_reissued_at":"2026-05-18T00:46:38.942636Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:46:38.942636Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Investigating the rotational evolution of very low-mass stars and brown dwarfs in young clusters using Monte Carlo simulations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"J. Bouvier, M. J. Vasconcelos","submitted_at":"2016-11-19T15:27:37Z","abstract_excerpt":"Context. Very low-mass (VLM) stars and brown dwarfs (BDs) present a different rotational behaviour from their solar mass counter-parts. Aims. We investigate the rotational evolution of young VLM stars and BDs using Monte Carlo simulations under the hypothesis of disk locking and stellar angular momentum conservation. Methods. We built a set of objects with masses ranging from 0.01 Mo to 0.4 Mo and considered models with single- and double- peaked initial period distributions with and without disk locking. An object is considered to be diskless when its mass accretion rate is below a given thre"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1611.06382","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":""},"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":"1611.06382","created_at":"2026-05-18T00:46:38.942742+00:00"},{"alias_kind":"arxiv_version","alias_value":"1611.06382v1","created_at":"2026-05-18T00:46:38.942742+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1611.06382","created_at":"2026-05-18T00:46:38.942742+00:00"},{"alias_kind":"pith_short_12","alias_value":"BGPSWLGAHAEW","created_at":"2026-05-18T12:30:07.202191+00:00"},{"alias_kind":"pith_short_16","alias_value":"BGPSWLGAHAEWEQYS","created_at":"2026-05-18T12:30:07.202191+00:00"},{"alias_kind":"pith_short_8","alias_value":"BGPSWLGA","created_at":"2026-05-18T12:30:07.202191+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/BGPSWLGAHAEWEQYS4TLS2AZO7D","json":"https://pith.science/pith/BGPSWLGAHAEWEQYS4TLS2AZO7D.json","graph_json":"https://pith.science/api/pith-number/BGPSWLGAHAEWEQYS4TLS2AZO7D/graph.json","events_json":"https://pith.science/api/pith-number/BGPSWLGAHAEWEQYS4TLS2AZO7D/events.json","paper":"https://pith.science/paper/BGPSWLGA"},"agent_actions":{"view_html":"https://pith.science/pith/BGPSWLGAHAEWEQYS4TLS2AZO7D","download_json":"https://pith.science/pith/BGPSWLGAHAEWEQYS4TLS2AZO7D.json","view_paper":"https://pith.science/paper/BGPSWLGA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1611.06382&json=true","fetch_graph":"https://pith.science/api/pith-number/BGPSWLGAHAEWEQYS4TLS2AZO7D/graph.json","fetch_events":"https://pith.science/api/pith-number/BGPSWLGAHAEWEQYS4TLS2AZO7D/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BGPSWLGAHAEWEQYS4TLS2AZO7D/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BGPSWLGAHAEWEQYS4TLS2AZO7D/action/storage_attestation","attest_author":"https://pith.science/pith/BGPSWLGAHAEWEQYS4TLS2AZO7D/action/author_attestation","sign_citation":"https://pith.science/pith/BGPSWLGAHAEWEQYS4TLS2AZO7D/action/citation_signature","submit_replication":"https://pith.science/pith/BGPSWLGAHAEWEQYS4TLS2AZO7D/action/replication_record"}},"created_at":"2026-05-18T00:46:38.942742+00:00","updated_at":"2026-05-18T00:46:38.942742+00:00"}