{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:1996:6VCTHFK4YRRYQKOQ6TYXM4IXKJ","short_pith_number":"pith:6VCTHFK4","schema_version":"1.0","canonical_sha256":"f54533955cc4638829d0f4f1767117526ea1bf40ab9beac16846c68cca0f7be2","source":{"kind":"arxiv","id":"astro-ph/9607083","version":1},"attestation_state":"computed","paper":{"title":"Residual gas expulsion from young globular clusters","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Simon P Goodwin","submitted_at":"1996-07-17T16:00:42Z","abstract_excerpt":"The results of N-body simulations of the expulsion of residual gas from young globular clusters are presented. Globular clusters with a variety of initial masses, Galactocentric radii, concentration and initial mass function slope with star formation efficiencies (SFEs) below 50% were investigated. The residual gas in the clusters was simply treated as an external potential acting upon the star particles which was reduced in a number of ways to simulate the loss of the gas. The states of the clusters after ~50 Myr was compared to the results of Chernoff & Shapiro (1987) in order to estimate if"},"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":"astro-ph/9607083","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"1996-07-17T16:00:42Z","cross_cats_sorted":[],"title_canon_sha256":"e64cfe186cb474f9347565c8de6b02431c033e930c839159a2f895e24a01fa07","abstract_canon_sha256":"83776c58721604a0d08bafddfe399e7de4dd1ba5e9a96bccbdecb912f0d190fd"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:40:19.728491Z","signature_b64":"rZYEO0HQrp/GndELpz7hfoCKNTJ+gFmjynIZ7PdG4ttnQRizUZU3Abq6uToGYnx7hm23kIwwGX4zTCD5QxpKDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f54533955cc4638829d0f4f1767117526ea1bf40ab9beac16846c68cca0f7be2","last_reissued_at":"2026-05-18T01:40:19.728070Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:40:19.728070Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Residual gas expulsion from young globular clusters","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Simon P Goodwin","submitted_at":"1996-07-17T16:00:42Z","abstract_excerpt":"The results of N-body simulations of the expulsion of residual gas from young globular clusters are presented. Globular clusters with a variety of initial masses, Galactocentric radii, concentration and initial mass function slope with star formation efficiencies (SFEs) below 50% were investigated. The residual gas in the clusters was simply treated as an external potential acting upon the star particles which was reduced in a number of ways to simulate the loss of the gas. The states of the clusters after ~50 Myr was compared to the results of Chernoff & Shapiro (1987) in order to estimate if"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/9607083","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":"astro-ph/9607083","created_at":"2026-05-18T01:40:19.728139+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/9607083v1","created_at":"2026-05-18T01:40:19.728139+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/9607083","created_at":"2026-05-18T01:40:19.728139+00:00"},{"alias_kind":"pith_short_12","alias_value":"6VCTHFK4YRRY","created_at":"2026-05-18T12:25:47.700082+00:00"},{"alias_kind":"pith_short_16","alias_value":"6VCTHFK4YRRYQKOQ","created_at":"2026-05-18T12:25:47.700082+00:00"},{"alias_kind":"pith_short_8","alias_value":"6VCTHFK4","created_at":"2026-05-18T12:25:47.700082+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/6VCTHFK4YRRYQKOQ6TYXM4IXKJ","json":"https://pith.science/pith/6VCTHFK4YRRYQKOQ6TYXM4IXKJ.json","graph_json":"https://pith.science/api/pith-number/6VCTHFK4YRRYQKOQ6TYXM4IXKJ/graph.json","events_json":"https://pith.science/api/pith-number/6VCTHFK4YRRYQKOQ6TYXM4IXKJ/events.json","paper":"https://pith.science/paper/6VCTHFK4"},"agent_actions":{"view_html":"https://pith.science/pith/6VCTHFK4YRRYQKOQ6TYXM4IXKJ","download_json":"https://pith.science/pith/6VCTHFK4YRRYQKOQ6TYXM4IXKJ.json","view_paper":"https://pith.science/paper/6VCTHFK4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/9607083&json=true","fetch_graph":"https://pith.science/api/pith-number/6VCTHFK4YRRYQKOQ6TYXM4IXKJ/graph.json","fetch_events":"https://pith.science/api/pith-number/6VCTHFK4YRRYQKOQ6TYXM4IXKJ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/6VCTHFK4YRRYQKOQ6TYXM4IXKJ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/6VCTHFK4YRRYQKOQ6TYXM4IXKJ/action/storage_attestation","attest_author":"https://pith.science/pith/6VCTHFK4YRRYQKOQ6TYXM4IXKJ/action/author_attestation","sign_citation":"https://pith.science/pith/6VCTHFK4YRRYQKOQ6TYXM4IXKJ/action/citation_signature","submit_replication":"https://pith.science/pith/6VCTHFK4YRRYQKOQ6TYXM4IXKJ/action/replication_record"}},"created_at":"2026-05-18T01:40:19.728139+00:00","updated_at":"2026-05-18T01:40:19.728139+00:00"}