{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:HD6RPIUCKQDCZNNHH4AKXNPUXS","short_pith_number":"pith:HD6RPIUC","schema_version":"1.0","canonical_sha256":"38fd17a28254062cb5a73f00abb5f4bc976d076646a6eac2f954ebb864fdecbb","source":{"kind":"arxiv","id":"1712.02908","version":1},"attestation_state":"computed","paper":{"title":"Two-dimensional modeling of density and thermal structure of dense circumstellar outflowing disks","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Achim Feldmeier, Ji\\v{r}\\'i Krti\\v{c}ka, Petr Kurf\\\"urst","submitted_at":"2017-12-08T01:35:35Z","abstract_excerpt":"Context. Evolution of massive stars is affected by a significant loss of mass either via (nearly) spherically symmetric stellar winds or by aspherical mass-loss mechanisms, namely the outflowing equatorial disks. However, the scenario that leads to the formation of a disk or rings of gas and dust around massive stars is still under debate. Aims. We study the hydrodynamic and thermal structure of optically thick, dense parts of outflowing circumstellar disks that may be formed around various types of critically rotating massive stars, for example, Be stars, B[e] supergiant (sgB[e]) stars or Pop"},"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":"1712.02908","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2017-12-08T01:35:35Z","cross_cats_sorted":[],"title_canon_sha256":"39ab10e257fddd4022d3f922432fa8e2522653622a343ecb1f664a2690224334","abstract_canon_sha256":"d703fa5929f07d1a4aa36c57198ccff86e1be56cd81805afa5503ae9b5224380"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:14:10.958946Z","signature_b64":"w7eX1b13eO7cAQDb7ivsnflqcpRcE1FHJEP/t+oQQ7nN1KWIt1AA6Cf1leEBg06YmGsBV6gJqJqLguAczN4pAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"38fd17a28254062cb5a73f00abb5f4bc976d076646a6eac2f954ebb864fdecbb","last_reissued_at":"2026-05-18T00:14:10.958237Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:14:10.958237Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Two-dimensional modeling of density and thermal structure of dense circumstellar outflowing disks","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Achim Feldmeier, Ji\\v{r}\\'i Krti\\v{c}ka, Petr Kurf\\\"urst","submitted_at":"2017-12-08T01:35:35Z","abstract_excerpt":"Context. Evolution of massive stars is affected by a significant loss of mass either via (nearly) spherically symmetric stellar winds or by aspherical mass-loss mechanisms, namely the outflowing equatorial disks. However, the scenario that leads to the formation of a disk or rings of gas and dust around massive stars is still under debate. Aims. We study the hydrodynamic and thermal structure of optically thick, dense parts of outflowing circumstellar disks that may be formed around various types of critically rotating massive stars, for example, Be stars, B[e] supergiant (sgB[e]) stars or Pop"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1712.02908","kind":"arxiv","version":1},"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":"1712.02908","created_at":"2026-05-18T00:14:10.958343+00:00"},{"alias_kind":"arxiv_version","alias_value":"1712.02908v1","created_at":"2026-05-18T00:14:10.958343+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1712.02908","created_at":"2026-05-18T00:14:10.958343+00:00"},{"alias_kind":"pith_short_12","alias_value":"HD6RPIUCKQDC","created_at":"2026-05-18T12:31:18.294218+00:00"},{"alias_kind":"pith_short_16","alias_value":"HD6RPIUCKQDCZNNH","created_at":"2026-05-18T12:31:18.294218+00:00"},{"alias_kind":"pith_short_8","alias_value":"HD6RPIUC","created_at":"2026-05-18T12:31:18.294218+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/HD6RPIUCKQDCZNNHH4AKXNPUXS","json":"https://pith.science/pith/HD6RPIUCKQDCZNNHH4AKXNPUXS.json","graph_json":"https://pith.science/api/pith-number/HD6RPIUCKQDCZNNHH4AKXNPUXS/graph.json","events_json":"https://pith.science/api/pith-number/HD6RPIUCKQDCZNNHH4AKXNPUXS/events.json","paper":"https://pith.science/paper/HD6RPIUC"},"agent_actions":{"view_html":"https://pith.science/pith/HD6RPIUCKQDCZNNHH4AKXNPUXS","download_json":"https://pith.science/pith/HD6RPIUCKQDCZNNHH4AKXNPUXS.json","view_paper":"https://pith.science/paper/HD6RPIUC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1712.02908&json=true","fetch_graph":"https://pith.science/api/pith-number/HD6RPIUCKQDCZNNHH4AKXNPUXS/graph.json","fetch_events":"https://pith.science/api/pith-number/HD6RPIUCKQDCZNNHH4AKXNPUXS/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HD6RPIUCKQDCZNNHH4AKXNPUXS/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HD6RPIUCKQDCZNNHH4AKXNPUXS/action/storage_attestation","attest_author":"https://pith.science/pith/HD6RPIUCKQDCZNNHH4AKXNPUXS/action/author_attestation","sign_citation":"https://pith.science/pith/HD6RPIUCKQDCZNNHH4AKXNPUXS/action/citation_signature","submit_replication":"https://pith.science/pith/HD6RPIUCKQDCZNNHH4AKXNPUXS/action/replication_record"}},"created_at":"2026-05-18T00:14:10.958343+00:00","updated_at":"2026-05-18T00:14:10.958343+00:00"}