{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2008:CDY3KINTDJGVQJEFN6MDSYRZ3L","short_pith_number":"pith:CDY3KINT","schema_version":"1.0","canonical_sha256":"10f1b521b31a4d5824856f98396239dad60d46d73e1c508cb74dfd1338cfd87c","source":{"kind":"arxiv","id":"0803.4215","version":2},"attestation_state":"computed","paper":{"title":"Feedback from galactic stellar bulges and hot gaseous haloes of galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"H. J. Mo, Q. Daniel Wang, Shikui Tang, Yu Lu","submitted_at":"2008-03-28T21:41:33Z","abstract_excerpt":"We demonstrate that the feedback from stellar bulges can play an essential role in shaping the halo gas of galaxies with substantial bulge components by conducting 1-D hydrodynamical simulations. The feedback model we consider consists of two distinct phases: 1) an early starburst during the bulge formation and 2) a subsequent long-lasting mass and energy injection from stellar winds of low-mass stars and Type Ia SNe. An energetic outward blastwave is initiated by the starburst and is maintained and enhanced by the long-lasting stellar feedback. For a MW-like galactic bulge, this blastwave swe"},"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":"0803.4215","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph","submitted_at":"2008-03-28T21:41:33Z","cross_cats_sorted":[],"title_canon_sha256":"a04c0a0f6b329757efeead6846d2110b8b6a04f77737db82ba4d733afe340e8a","abstract_canon_sha256":"90bf418badbeba52aff29d2c79230fb1b73ed66c3d56a07fab82b4d8c87a304f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:35:23.001668Z","signature_b64":"dMHpizAIjm03JS/TE52pjzSwf0SP7K8gC2HshcqhwlxBcKQHBj0ikXm9mkFqksfV1hvvAm73n3JDIkxtUAHZDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"10f1b521b31a4d5824856f98396239dad60d46d73e1c508cb74dfd1338cfd87c","last_reissued_at":"2026-05-18T02:35:23.001271Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:35:23.001271Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Feedback from galactic stellar bulges and hot gaseous haloes of galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"H. J. Mo, Q. Daniel Wang, Shikui Tang, Yu Lu","submitted_at":"2008-03-28T21:41:33Z","abstract_excerpt":"We demonstrate that the feedback from stellar bulges can play an essential role in shaping the halo gas of galaxies with substantial bulge components by conducting 1-D hydrodynamical simulations. The feedback model we consider consists of two distinct phases: 1) an early starburst during the bulge formation and 2) a subsequent long-lasting mass and energy injection from stellar winds of low-mass stars and Type Ia SNe. An energetic outward blastwave is initiated by the starburst and is maintained and enhanced by the long-lasting stellar feedback. For a MW-like galactic bulge, this blastwave swe"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0803.4215","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":"0803.4215","created_at":"2026-05-18T02:35:23.001339+00:00"},{"alias_kind":"arxiv_version","alias_value":"0803.4215v2","created_at":"2026-05-18T02:35:23.001339+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0803.4215","created_at":"2026-05-18T02:35:23.001339+00:00"},{"alias_kind":"pith_short_12","alias_value":"CDY3KINTDJGV","created_at":"2026-05-18T12:25:57.157939+00:00"},{"alias_kind":"pith_short_16","alias_value":"CDY3KINTDJGVQJEF","created_at":"2026-05-18T12:25:57.157939+00:00"},{"alias_kind":"pith_short_8","alias_value":"CDY3KINT","created_at":"2026-05-18T12:25:57.157939+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/CDY3KINTDJGVQJEFN6MDSYRZ3L","json":"https://pith.science/pith/CDY3KINTDJGVQJEFN6MDSYRZ3L.json","graph_json":"https://pith.science/api/pith-number/CDY3KINTDJGVQJEFN6MDSYRZ3L/graph.json","events_json":"https://pith.science/api/pith-number/CDY3KINTDJGVQJEFN6MDSYRZ3L/events.json","paper":"https://pith.science/paper/CDY3KINT"},"agent_actions":{"view_html":"https://pith.science/pith/CDY3KINTDJGVQJEFN6MDSYRZ3L","download_json":"https://pith.science/pith/CDY3KINTDJGVQJEFN6MDSYRZ3L.json","view_paper":"https://pith.science/paper/CDY3KINT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0803.4215&json=true","fetch_graph":"https://pith.science/api/pith-number/CDY3KINTDJGVQJEFN6MDSYRZ3L/graph.json","fetch_events":"https://pith.science/api/pith-number/CDY3KINTDJGVQJEFN6MDSYRZ3L/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CDY3KINTDJGVQJEFN6MDSYRZ3L/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CDY3KINTDJGVQJEFN6MDSYRZ3L/action/storage_attestation","attest_author":"https://pith.science/pith/CDY3KINTDJGVQJEFN6MDSYRZ3L/action/author_attestation","sign_citation":"https://pith.science/pith/CDY3KINTDJGVQJEFN6MDSYRZ3L/action/citation_signature","submit_replication":"https://pith.science/pith/CDY3KINTDJGVQJEFN6MDSYRZ3L/action/replication_record"}},"created_at":"2026-05-18T02:35:23.001339+00:00","updated_at":"2026-05-18T02:35:23.001339+00:00"}