{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:FSOXRSFWZZBNVNBOJSBVA5ODPQ","short_pith_number":"pith:FSOXRSFW","schema_version":"1.0","canonical_sha256":"2c9d78c8b6ce42dab42e4c835075c37c33af894d4690f2b11bc1087a550d934b","source":{"kind":"arxiv","id":"1706.00118","version":1},"attestation_state":"computed","paper":{"title":"High-Mass Star and Massive Cluster Formation in the Milky Way","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.GA","authors_text":"Fabien Louvet, Frederique Motte, Sylvain Bontemps","submitted_at":"2017-05-31T23:02:09Z","abstract_excerpt":"This review examines the state-of-the-art knowledge of high-mass star and massive cluster formation, gained from ambitious observational surveys, which acknowledge the multi-scale characteristics of these processes. After a brief overview of theoretical models and main open issues, we present observational searches for the evolutionary phases of high-mass star formation, first among high-luminosity sources and more recently among young massive protostars and the elusive high-mass prestellar cores. We then introduce the most likely evolutionary scenario for high-mass star formation, which empha"},"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":"1706.00118","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-05-31T23:02:09Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"10355e3f929445cd85c8775abb76e891fbaa1cdd1efd8cc27f3fe0e9e590da45","abstract_canon_sha256":"a3dc63f2c7bc1a0088b389832d3618113e1161f2c7c224fb88587eb90b7ad997"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:20:52.278262Z","signature_b64":"MprCKRaSfbitl/ffBDheYiuvAmv7nzZbBEl1UvvKH7g+j4JFrZ1YKaibX9ZVNDIbzXFQU+mJYCrOzWLAzMEFAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2c9d78c8b6ce42dab42e4c835075c37c33af894d4690f2b11bc1087a550d934b","last_reissued_at":"2026-05-18T00:20:52.277751Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:20:52.277751Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"High-Mass Star and Massive Cluster Formation in the Milky Way","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.GA","authors_text":"Fabien Louvet, Frederique Motte, Sylvain Bontemps","submitted_at":"2017-05-31T23:02:09Z","abstract_excerpt":"This review examines the state-of-the-art knowledge of high-mass star and massive cluster formation, gained from ambitious observational surveys, which acknowledge the multi-scale characteristics of these processes. After a brief overview of theoretical models and main open issues, we present observational searches for the evolutionary phases of high-mass star formation, first among high-luminosity sources and more recently among young massive protostars and the elusive high-mass prestellar cores. We then introduce the most likely evolutionary scenario for high-mass star formation, which empha"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1706.00118","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":"1706.00118","created_at":"2026-05-18T00:20:52.277833+00:00"},{"alias_kind":"arxiv_version","alias_value":"1706.00118v1","created_at":"2026-05-18T00:20:52.277833+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1706.00118","created_at":"2026-05-18T00:20:52.277833+00:00"},{"alias_kind":"pith_short_12","alias_value":"FSOXRSFWZZBN","created_at":"2026-05-18T12:31:15.632608+00:00"},{"alias_kind":"pith_short_16","alias_value":"FSOXRSFWZZBNVNBO","created_at":"2026-05-18T12:31:15.632608+00:00"},{"alias_kind":"pith_short_8","alias_value":"FSOXRSFW","created_at":"2026-05-18T12:31:15.632608+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/FSOXRSFWZZBNVNBOJSBVA5ODPQ","json":"https://pith.science/pith/FSOXRSFWZZBNVNBOJSBVA5ODPQ.json","graph_json":"https://pith.science/api/pith-number/FSOXRSFWZZBNVNBOJSBVA5ODPQ/graph.json","events_json":"https://pith.science/api/pith-number/FSOXRSFWZZBNVNBOJSBVA5ODPQ/events.json","paper":"https://pith.science/paper/FSOXRSFW"},"agent_actions":{"view_html":"https://pith.science/pith/FSOXRSFWZZBNVNBOJSBVA5ODPQ","download_json":"https://pith.science/pith/FSOXRSFWZZBNVNBOJSBVA5ODPQ.json","view_paper":"https://pith.science/paper/FSOXRSFW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1706.00118&json=true","fetch_graph":"https://pith.science/api/pith-number/FSOXRSFWZZBNVNBOJSBVA5ODPQ/graph.json","fetch_events":"https://pith.science/api/pith-number/FSOXRSFWZZBNVNBOJSBVA5ODPQ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FSOXRSFWZZBNVNBOJSBVA5ODPQ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FSOXRSFWZZBNVNBOJSBVA5ODPQ/action/storage_attestation","attest_author":"https://pith.science/pith/FSOXRSFWZZBNVNBOJSBVA5ODPQ/action/author_attestation","sign_citation":"https://pith.science/pith/FSOXRSFWZZBNVNBOJSBVA5ODPQ/action/citation_signature","submit_replication":"https://pith.science/pith/FSOXRSFWZZBNVNBOJSBVA5ODPQ/action/replication_record"}},"created_at":"2026-05-18T00:20:52.277833+00:00","updated_at":"2026-05-18T00:20:52.277833+00:00"}