{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:JBBLVG2BJ4VU7B2M5TYQKVI52J","short_pith_number":"pith:JBBLVG2B","schema_version":"1.0","canonical_sha256":"4842ba9b414f2b4f874cecf105551dd27bd06b3a7423a5044bb4c514ddc131db","source":{"kind":"arxiv","id":"1706.00477","version":1},"attestation_state":"computed","paper":{"title":"Simulating radiative feedback and star cluster formation in GMCs: II. Mass dependence of cloud destruction and cluster properties","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Corey Howard, Ralph Pudritz, William Harris","submitted_at":"2017-06-01T20:00:00Z","abstract_excerpt":"The process of radiative feedback in Giant Molecular Clouds (GMCs) is an important mechanism for limiting star cluster formation through the heating and ionization of the surrounding gas. We explore the degree to which radiative feedback affects early ($\\lesssim$5 Myr) cluster formation in GMCs having masses that range from 10$^{4-6}$ M$_{\\odot}$ using the FLASH code. The inclusion of radiative feedback lowers the efficiency of cluster formation by 20-50\\% relative to hydrodynamic simulations. Two models in particular --- 5$\\times$10$^4$ and 10$^5$ M$_{\\odot}$ --- show the largest suppression "},"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":"1706.00477","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-06-01T20:00:00Z","cross_cats_sorted":[],"title_canon_sha256":"b5fcd237c3babda978cc6caf4aecf096205ea993564c0401eed5cb48903c8641","abstract_canon_sha256":"f6195caeb4229f7b84fb9d95c49495da18c17575cd403c4174d1b7917b802cae"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:39:34.359706Z","signature_b64":"ii969lphDDb0jWarLI4vlOoC4OazMPhQy5I+I3v+st2q964xvnWr8N26eZS+7nes6Hld1FrhSNaZVeSLFQB+BQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4842ba9b414f2b4f874cecf105551dd27bd06b3a7423a5044bb4c514ddc131db","last_reissued_at":"2026-05-18T00:39:34.359053Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:39:34.359053Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Simulating radiative feedback and star cluster formation in GMCs: II. Mass dependence of cloud destruction and cluster properties","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Corey Howard, Ralph Pudritz, William Harris","submitted_at":"2017-06-01T20:00:00Z","abstract_excerpt":"The process of radiative feedback in Giant Molecular Clouds (GMCs) is an important mechanism for limiting star cluster formation through the heating and ionization of the surrounding gas. We explore the degree to which radiative feedback affects early ($\\lesssim$5 Myr) cluster formation in GMCs having masses that range from 10$^{4-6}$ M$_{\\odot}$ using the FLASH code. The inclusion of radiative feedback lowers the efficiency of cluster formation by 20-50\\% relative to hydrodynamic simulations. Two models in particular --- 5$\\times$10$^4$ and 10$^5$ M$_{\\odot}$ --- show the largest suppression "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1706.00477","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":"1706.00477","created_at":"2026-05-18T00:39:34.359151+00:00"},{"alias_kind":"arxiv_version","alias_value":"1706.00477v1","created_at":"2026-05-18T00:39:34.359151+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1706.00477","created_at":"2026-05-18T00:39:34.359151+00:00"},{"alias_kind":"pith_short_12","alias_value":"JBBLVG2BJ4VU","created_at":"2026-05-18T12:31:21.493067+00:00"},{"alias_kind":"pith_short_16","alias_value":"JBBLVG2BJ4VU7B2M","created_at":"2026-05-18T12:31:21.493067+00:00"},{"alias_kind":"pith_short_8","alias_value":"JBBLVG2B","created_at":"2026-05-18T12:31:21.493067+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/JBBLVG2BJ4VU7B2M5TYQKVI52J","json":"https://pith.science/pith/JBBLVG2BJ4VU7B2M5TYQKVI52J.json","graph_json":"https://pith.science/api/pith-number/JBBLVG2BJ4VU7B2M5TYQKVI52J/graph.json","events_json":"https://pith.science/api/pith-number/JBBLVG2BJ4VU7B2M5TYQKVI52J/events.json","paper":"https://pith.science/paper/JBBLVG2B"},"agent_actions":{"view_html":"https://pith.science/pith/JBBLVG2BJ4VU7B2M5TYQKVI52J","download_json":"https://pith.science/pith/JBBLVG2BJ4VU7B2M5TYQKVI52J.json","view_paper":"https://pith.science/paper/JBBLVG2B","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1706.00477&json=true","fetch_graph":"https://pith.science/api/pith-number/JBBLVG2BJ4VU7B2M5TYQKVI52J/graph.json","fetch_events":"https://pith.science/api/pith-number/JBBLVG2BJ4VU7B2M5TYQKVI52J/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JBBLVG2BJ4VU7B2M5TYQKVI52J/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JBBLVG2BJ4VU7B2M5TYQKVI52J/action/storage_attestation","attest_author":"https://pith.science/pith/JBBLVG2BJ4VU7B2M5TYQKVI52J/action/author_attestation","sign_citation":"https://pith.science/pith/JBBLVG2BJ4VU7B2M5TYQKVI52J/action/citation_signature","submit_replication":"https://pith.science/pith/JBBLVG2BJ4VU7B2M5TYQKVI52J/action/replication_record"}},"created_at":"2026-05-18T00:39:34.359151+00:00","updated_at":"2026-05-18T00:39:34.359151+00:00"}