{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:5NDBK6ZOPTKEUR4AXB5UEQK4IA","short_pith_number":"pith:5NDBK6ZO","schema_version":"1.0","canonical_sha256":"eb46157b2e7cd44a4780b87b42415c403e705128125f84aaef4ef3375e8f7400","source":{"kind":"arxiv","id":"1301.0841","version":2},"attestation_state":"computed","paper":{"title":"Resolving The Generation of Starburst Winds in Galaxy Mergers","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"(2) UCSD, (3) CITA, (4) Harvard, (5) Steward, (6) Heidelberg), Christopher C. Hayward (6) ((1) Caltech/Berkeley, Desika Narayanan (5), Dusan Keres (2), Lars Hernquist (4), Norman Murray (3), Philip F. Hopkins (1)","submitted_at":"2013-01-04T21:54:19Z","abstract_excerpt":"We study galaxy super-winds driven in major mergers, using pc-resolution simulations with detailed models for stellar feedback that can self-consistently follow the formation/destruction of GMCs and generation of winds. The models include molecular cooling, star formation at high densities in GMCs, and gas recycling and feedback from SNe (I&II), stellar winds, and radiation pressure. We study mergers of systems from SMC-like dwarfs and Milky Way analogues to z~2 starburst disks. Multi-phase super-winds are generated in all passages, with outflow rates up to ~1000 M_sun/yr. However, the wind ma"},"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":"1301.0841","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-01-04T21:54:19Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"61fb758782d504e27d99757e962bfcd6819a4ba17c9b454ab98921e81998a3f9","abstract_canon_sha256":"b1e3e4a607617bc141c224a0e34020701c9ffcddb0d0a1aaa1f277f75b54c514"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:37:52.220577Z","signature_b64":"fkFObmyfYgKj0q/kStUoUVnWwFA+SQmjEwBDumVQx+1GkYB+njUQ4SvyVnEuMSlW5UIqTiDOaL19LQW80LYkBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"eb46157b2e7cd44a4780b87b42415c403e705128125f84aaef4ef3375e8f7400","last_reissued_at":"2026-05-18T02:37:52.219981Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:37:52.219981Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Resolving The Generation of Starburst Winds in Galaxy Mergers","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"(2) UCSD, (3) CITA, (4) Harvard, (5) Steward, (6) Heidelberg), Christopher C. Hayward (6) ((1) Caltech/Berkeley, Desika Narayanan (5), Dusan Keres (2), Lars Hernquist (4), Norman Murray (3), Philip F. Hopkins (1)","submitted_at":"2013-01-04T21:54:19Z","abstract_excerpt":"We study galaxy super-winds driven in major mergers, using pc-resolution simulations with detailed models for stellar feedback that can self-consistently follow the formation/destruction of GMCs and generation of winds. The models include molecular cooling, star formation at high densities in GMCs, and gas recycling and feedback from SNe (I&II), stellar winds, and radiation pressure. We study mergers of systems from SMC-like dwarfs and Milky Way analogues to z~2 starburst disks. Multi-phase super-winds are generated in all passages, with outflow rates up to ~1000 M_sun/yr. However, the wind ma"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1301.0841","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":""},"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":"1301.0841","created_at":"2026-05-18T02:37:52.220064+00:00"},{"alias_kind":"arxiv_version","alias_value":"1301.0841v2","created_at":"2026-05-18T02:37:52.220064+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1301.0841","created_at":"2026-05-18T02:37:52.220064+00:00"},{"alias_kind":"pith_short_12","alias_value":"5NDBK6ZOPTKE","created_at":"2026-05-18T12:27:34.582898+00:00"},{"alias_kind":"pith_short_16","alias_value":"5NDBK6ZOPTKEUR4A","created_at":"2026-05-18T12:27:34.582898+00:00"},{"alias_kind":"pith_short_8","alias_value":"5NDBK6ZO","created_at":"2026-05-18T12:27:34.582898+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/5NDBK6ZOPTKEUR4AXB5UEQK4IA","json":"https://pith.science/pith/5NDBK6ZOPTKEUR4AXB5UEQK4IA.json","graph_json":"https://pith.science/api/pith-number/5NDBK6ZOPTKEUR4AXB5UEQK4IA/graph.json","events_json":"https://pith.science/api/pith-number/5NDBK6ZOPTKEUR4AXB5UEQK4IA/events.json","paper":"https://pith.science/paper/5NDBK6ZO"},"agent_actions":{"view_html":"https://pith.science/pith/5NDBK6ZOPTKEUR4AXB5UEQK4IA","download_json":"https://pith.science/pith/5NDBK6ZOPTKEUR4AXB5UEQK4IA.json","view_paper":"https://pith.science/paper/5NDBK6ZO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1301.0841&json=true","fetch_graph":"https://pith.science/api/pith-number/5NDBK6ZOPTKEUR4AXB5UEQK4IA/graph.json","fetch_events":"https://pith.science/api/pith-number/5NDBK6ZOPTKEUR4AXB5UEQK4IA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5NDBK6ZOPTKEUR4AXB5UEQK4IA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5NDBK6ZOPTKEUR4AXB5UEQK4IA/action/storage_attestation","attest_author":"https://pith.science/pith/5NDBK6ZOPTKEUR4AXB5UEQK4IA/action/author_attestation","sign_citation":"https://pith.science/pith/5NDBK6ZOPTKEUR4AXB5UEQK4IA/action/citation_signature","submit_replication":"https://pith.science/pith/5NDBK6ZOPTKEUR4AXB5UEQK4IA/action/replication_record"}},"created_at":"2026-05-18T02:37:52.220064+00:00","updated_at":"2026-05-18T02:37:52.220064+00:00"}