{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:5NZWDAGBA3HFOJPEUYOFH6KQZL","short_pith_number":"pith:5NZWDAGB","schema_version":"1.0","canonical_sha256":"eb736180c106ce5725e4a61c53f950caff4cd92f377751e93bdbe71c4cd76726","source":{"kind":"arxiv","id":"1708.02646","version":2},"attestation_state":"computed","paper":{"title":"Numerical Simulations of Supernova Remnant Evolution in a Cloudy Interstellar Medium","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"Adam Foster, Henry D. Winter, Hiroya Yamaguchi, John C. Raymond, Jonathan D. Slavin, Patrick O. Slane, Randall K. Smith","submitted_at":"2017-08-08T20:35:47Z","abstract_excerpt":"The mixed morphology class of supernova remnants has centrally peaked X-ray emission along with a shell-like morphology in radio emission. White & Long proposed that these remnants are evolving in a cloudy medium wherein the clouds are evaporated via thermal conduction once being overrun by the expanding shock. Their analytical model made detailed predictions regarding temperature, density and emission profiles as well as shock evolution. We present numerical hydrodynamical models in 2D and 3D including thermal conduction, testing the White & Long model and presenting results for the evolution"},"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":"1708.02646","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-08-08T20:35:47Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"9a85d67c798f29aff73352e5c838812fd0081379f185f0438381d560ac7e3290","abstract_canon_sha256":"d19af528e6c6b63df437e66d589d0732a558ae72461f17e096005ec8edd13831"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:35:30.647195Z","signature_b64":"eVMgRu4R1DeurFC2ovOcNy0t0zqmnFqENtQhPLVYX92Rj/R0/7QVO070TH81HhcYJuUgMBjtNTcj7sS7szilCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"eb736180c106ce5725e4a61c53f950caff4cd92f377751e93bdbe71c4cd76726","last_reissued_at":"2026-05-18T00:35:30.646652Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:35:30.646652Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Numerical Simulations of Supernova Remnant Evolution in a Cloudy Interstellar Medium","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"Adam Foster, Henry D. Winter, Hiroya Yamaguchi, John C. Raymond, Jonathan D. Slavin, Patrick O. Slane, Randall K. Smith","submitted_at":"2017-08-08T20:35:47Z","abstract_excerpt":"The mixed morphology class of supernova remnants has centrally peaked X-ray emission along with a shell-like morphology in radio emission. White & Long proposed that these remnants are evolving in a cloudy medium wherein the clouds are evaporated via thermal conduction once being overrun by the expanding shock. Their analytical model made detailed predictions regarding temperature, density and emission profiles as well as shock evolution. We present numerical hydrodynamical models in 2D and 3D including thermal conduction, testing the White & Long model and presenting results for the evolution"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1708.02646","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":"1708.02646","created_at":"2026-05-18T00:35:30.646743+00:00"},{"alias_kind":"arxiv_version","alias_value":"1708.02646v2","created_at":"2026-05-18T00:35:30.646743+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1708.02646","created_at":"2026-05-18T00:35:30.646743+00:00"},{"alias_kind":"pith_short_12","alias_value":"5NZWDAGBA3HF","created_at":"2026-05-18T12:31:00.734936+00:00"},{"alias_kind":"pith_short_16","alias_value":"5NZWDAGBA3HFOJPE","created_at":"2026-05-18T12:31:00.734936+00:00"},{"alias_kind":"pith_short_8","alias_value":"5NZWDAGB","created_at":"2026-05-18T12:31:00.734936+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/5NZWDAGBA3HFOJPEUYOFH6KQZL","json":"https://pith.science/pith/5NZWDAGBA3HFOJPEUYOFH6KQZL.json","graph_json":"https://pith.science/api/pith-number/5NZWDAGBA3HFOJPEUYOFH6KQZL/graph.json","events_json":"https://pith.science/api/pith-number/5NZWDAGBA3HFOJPEUYOFH6KQZL/events.json","paper":"https://pith.science/paper/5NZWDAGB"},"agent_actions":{"view_html":"https://pith.science/pith/5NZWDAGBA3HFOJPEUYOFH6KQZL","download_json":"https://pith.science/pith/5NZWDAGBA3HFOJPEUYOFH6KQZL.json","view_paper":"https://pith.science/paper/5NZWDAGB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1708.02646&json=true","fetch_graph":"https://pith.science/api/pith-number/5NZWDAGBA3HFOJPEUYOFH6KQZL/graph.json","fetch_events":"https://pith.science/api/pith-number/5NZWDAGBA3HFOJPEUYOFH6KQZL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5NZWDAGBA3HFOJPEUYOFH6KQZL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5NZWDAGBA3HFOJPEUYOFH6KQZL/action/storage_attestation","attest_author":"https://pith.science/pith/5NZWDAGBA3HFOJPEUYOFH6KQZL/action/author_attestation","sign_citation":"https://pith.science/pith/5NZWDAGBA3HFOJPEUYOFH6KQZL/action/citation_signature","submit_replication":"https://pith.science/pith/5NZWDAGBA3HFOJPEUYOFH6KQZL/action/replication_record"}},"created_at":"2026-05-18T00:35:30.646743+00:00","updated_at":"2026-05-18T00:35:30.646743+00:00"}