{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:2X6AA3FHKX4K2P6TSSREQI3I6V","short_pith_number":"pith:2X6AA3FH","schema_version":"1.0","canonical_sha256":"d5fc006ca755f8ad3fd394a2482368f55c49b2bfced4b8f178964e725b67ca91","source":{"kind":"arxiv","id":"1010.1051","version":3},"attestation_state":"computed","paper":{"title":"Galactic Coronae in the Intracluster Environment: Semi-confined Stellar-feedback-driven Outflows","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Q. Daniel Wang, Zhankui Lu","submitted_at":"2010-10-06T03:01:56Z","abstract_excerpt":"Recently X-ray observations have shown the common presence of compact galactic coronae around intermediate-mass spheroid galaxies embedded in the intracluster/intragroup medium (ICM). We conduct 2-D hydrodynamic simulations to study the quasi-steady-state properties of such coronae as the natural products of the ongoing distributed stellar feedback semi-confined by the thermal and ram pressures of the ICM. We find that the temperature of a simulated corona depends primarily on the specific energy of the feedback, consistent with the lack of the correlation between the observed hot gas temperat"},"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":"1010.1051","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2010-10-06T03:01:56Z","cross_cats_sorted":[],"title_canon_sha256":"0ac69ddf67fadc929d5c6d7711c556a2b531b10fe31b2a02f7cfe62964aa0bcb","abstract_canon_sha256":"a096589cd0a6044a35bafcb943308a2d8d26ea3f598c4c6e7dc57304c8df008d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:05:10.811167Z","signature_b64":"dbBUjg82CVpOHr5XCnYHuo9/FOoOhi4M5fh0Bcl6U+6EvQ5AtaqJYqtE83lT1rZfy/DaIPm++E1JkRdGDAq/Cw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d5fc006ca755f8ad3fd394a2482368f55c49b2bfced4b8f178964e725b67ca91","last_reissued_at":"2026-05-18T02:05:10.810418Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:05:10.810418Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Galactic Coronae in the Intracluster Environment: Semi-confined Stellar-feedback-driven Outflows","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Q. Daniel Wang, Zhankui Lu","submitted_at":"2010-10-06T03:01:56Z","abstract_excerpt":"Recently X-ray observations have shown the common presence of compact galactic coronae around intermediate-mass spheroid galaxies embedded in the intracluster/intragroup medium (ICM). We conduct 2-D hydrodynamic simulations to study the quasi-steady-state properties of such coronae as the natural products of the ongoing distributed stellar feedback semi-confined by the thermal and ram pressures of the ICM. We find that the temperature of a simulated corona depends primarily on the specific energy of the feedback, consistent with the lack of the correlation between the observed hot gas temperat"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1010.1051","kind":"arxiv","version":3},"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":"1010.1051","created_at":"2026-05-18T02:05:10.810504+00:00"},{"alias_kind":"arxiv_version","alias_value":"1010.1051v3","created_at":"2026-05-18T02:05:10.810504+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1010.1051","created_at":"2026-05-18T02:05:10.810504+00:00"},{"alias_kind":"pith_short_12","alias_value":"2X6AA3FHKX4K","created_at":"2026-05-18T12:26:03.138858+00:00"},{"alias_kind":"pith_short_16","alias_value":"2X6AA3FHKX4K2P6T","created_at":"2026-05-18T12:26:03.138858+00:00"},{"alias_kind":"pith_short_8","alias_value":"2X6AA3FH","created_at":"2026-05-18T12:26:03.138858+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/2X6AA3FHKX4K2P6TSSREQI3I6V","json":"https://pith.science/pith/2X6AA3FHKX4K2P6TSSREQI3I6V.json","graph_json":"https://pith.science/api/pith-number/2X6AA3FHKX4K2P6TSSREQI3I6V/graph.json","events_json":"https://pith.science/api/pith-number/2X6AA3FHKX4K2P6TSSREQI3I6V/events.json","paper":"https://pith.science/paper/2X6AA3FH"},"agent_actions":{"view_html":"https://pith.science/pith/2X6AA3FHKX4K2P6TSSREQI3I6V","download_json":"https://pith.science/pith/2X6AA3FHKX4K2P6TSSREQI3I6V.json","view_paper":"https://pith.science/paper/2X6AA3FH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1010.1051&json=true","fetch_graph":"https://pith.science/api/pith-number/2X6AA3FHKX4K2P6TSSREQI3I6V/graph.json","fetch_events":"https://pith.science/api/pith-number/2X6AA3FHKX4K2P6TSSREQI3I6V/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2X6AA3FHKX4K2P6TSSREQI3I6V/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2X6AA3FHKX4K2P6TSSREQI3I6V/action/storage_attestation","attest_author":"https://pith.science/pith/2X6AA3FHKX4K2P6TSSREQI3I6V/action/author_attestation","sign_citation":"https://pith.science/pith/2X6AA3FHKX4K2P6TSSREQI3I6V/action/citation_signature","submit_replication":"https://pith.science/pith/2X6AA3FHKX4K2P6TSSREQI3I6V/action/replication_record"}},"created_at":"2026-05-18T02:05:10.810504+00:00","updated_at":"2026-05-18T02:05:10.810504+00:00"}