{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:3GZEINEFAG7WGACRZHGG3WEUZH","short_pith_number":"pith:3GZEINEF","schema_version":"1.0","canonical_sha256":"d9b244348501bf630051c9cc6dd894c9dbbedb8c2f7a383ce2e7960863a21497","source":{"kind":"arxiv","id":"1701.09062","version":2},"attestation_state":"computed","paper":{"title":"Galactic Winds and the Role Played by Massive Stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Timothy M. Heckman, Todd A. Thompson","submitted_at":"2017-01-31T14:44:17Z","abstract_excerpt":"Galactic winds from star-forming galaxies play at key role in the evolution of galaxies and the inter-galactic medium. They transport metals out of galaxies, chemically-enriching the inter-galactic medium and modifying the chemical evolution of galaxies. They affect the surrounding inter-stellar and circum-galactic media, thereby influencing the growth of galaxies through gas accretion and star-formation. In this contribution we first summarize the physical mechanisms by which the momentum and energy output from a population of massive stars and associated supernovae can drive galactic winds. "},"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":"1701.09062","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-01-31T14:44:17Z","cross_cats_sorted":[],"title_canon_sha256":"7ed8deb4d011c9128c86346aef6d2ffb4ee1c7bea70e977ece8881f9d71924e1","abstract_canon_sha256":"77930440ca997a506a96e036d6e01c271297ad32fdcfa25ca24f238634aba9a0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:16:29.191512Z","signature_b64":"pMpRKYZmgm0RYQH0xNh8B3MB+tdJ/JN1s4+kL52nWafdsOChn8abkyAl/dIWMHktGh1Mi/Smtu4+QeLiLQwxCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d9b244348501bf630051c9cc6dd894c9dbbedb8c2f7a383ce2e7960863a21497","last_reissued_at":"2026-07-05T00:16:29.191001Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:16:29.191001Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Galactic Winds and the Role Played by Massive Stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Timothy M. Heckman, Todd A. Thompson","submitted_at":"2017-01-31T14:44:17Z","abstract_excerpt":"Galactic winds from star-forming galaxies play at key role in the evolution of galaxies and the inter-galactic medium. They transport metals out of galaxies, chemically-enriching the inter-galactic medium and modifying the chemical evolution of galaxies. They affect the surrounding inter-stellar and circum-galactic media, thereby influencing the growth of galaxies through gas accretion and star-formation. In this contribution we first summarize the physical mechanisms by which the momentum and energy output from a population of massive stars and associated supernovae can drive galactic winds. "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1701.09062","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/1701.09062/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"1701.09062","created_at":"2026-07-05T00:16:29.191069+00:00"},{"alias_kind":"arxiv_version","alias_value":"1701.09062v2","created_at":"2026-07-05T00:16:29.191069+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1701.09062","created_at":"2026-07-05T00:16:29.191069+00:00"},{"alias_kind":"pith_short_12","alias_value":"3GZEINEFAG7W","created_at":"2026-07-05T00:16:29.191069+00:00"},{"alias_kind":"pith_short_16","alias_value":"3GZEINEFAG7WGACR","created_at":"2026-07-05T00:16:29.191069+00:00"},{"alias_kind":"pith_short_8","alias_value":"3GZEINEF","created_at":"2026-07-05T00:16:29.191069+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.08264","citing_title":"Subaru meets JWST: A Direct Measurement of Ly$\\boldsymbol{\\alpha}$ Escape Fraction at $\\boldsymbol{z\\simeq6.2}$ with Dual Narrow-Band Imaging","ref_index":58,"is_internal_anchor":true},{"citing_arxiv_id":"2507.16115","citing_title":"Simba Simulation: The Effect of Feedback Physics on Matter Distribution in the Cosmic Web","ref_index":55,"is_internal_anchor":false},{"citing_arxiv_id":"2605.03016","citing_title":"Resolving the Multiphase Outflow, Shock Signatures, and PAHs in the AGN-Starburst Composite ULIRG F10565+2448 with JWST MIRI/MRS","ref_index":28,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/3GZEINEFAG7WGACRZHGG3WEUZH","json":"https://pith.science/pith/3GZEINEFAG7WGACRZHGG3WEUZH.json","graph_json":"https://pith.science/api/pith-number/3GZEINEFAG7WGACRZHGG3WEUZH/graph.json","events_json":"https://pith.science/api/pith-number/3GZEINEFAG7WGACRZHGG3WEUZH/events.json","paper":"https://pith.science/paper/3GZEINEF"},"agent_actions":{"view_html":"https://pith.science/pith/3GZEINEFAG7WGACRZHGG3WEUZH","download_json":"https://pith.science/pith/3GZEINEFAG7WGACRZHGG3WEUZH.json","view_paper":"https://pith.science/paper/3GZEINEF","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1701.09062&json=true","fetch_graph":"https://pith.science/api/pith-number/3GZEINEFAG7WGACRZHGG3WEUZH/graph.json","fetch_events":"https://pith.science/api/pith-number/3GZEINEFAG7WGACRZHGG3WEUZH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3GZEINEFAG7WGACRZHGG3WEUZH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3GZEINEFAG7WGACRZHGG3WEUZH/action/storage_attestation","attest_author":"https://pith.science/pith/3GZEINEFAG7WGACRZHGG3WEUZH/action/author_attestation","sign_citation":"https://pith.science/pith/3GZEINEFAG7WGACRZHGG3WEUZH/action/citation_signature","submit_replication":"https://pith.science/pith/3GZEINEFAG7WGACRZHGG3WEUZH/action/replication_record"}},"created_at":"2026-07-05T00:16:29.191069+00:00","updated_at":"2026-07-05T00:16:29.191069+00:00"}