{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:NOJDFAJKPFIHM2SQTBV2CWSEBG","short_pith_number":"pith:NOJDFAJK","schema_version":"1.0","canonical_sha256":"6b9232812a7950766a50986ba15a44099de34c0d5b66eb5afca115aef834bc68","source":{"kind":"arxiv","id":"1405.1960","version":2},"attestation_state":"computed","paper":{"title":"An interferometric study of the post-AGB binary 89 Herculis. II Radiative transfer models of the circumbinary disk","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"C. Gielen, G. D. Mulders, H. Van Winckel, J. Menu, M. Hillen, M. Min, S. Regibo, T. Verhoelst, T. Wevers","submitted_at":"2014-05-08T15:17:34Z","abstract_excerpt":"The presence of disks and outflows is widespread among post-AGB binaries. In the first paper of this series, a surprisingly large fraction of optical light was found to be resolved in the 89 Her post-AGB system. The data showed this flux to arise from close to the central binary. Scattering off the inner rim of the circumbinary disk, or in a dusty outflow were suggested as two possible origins. With detailed dust radiative transfer models of the disk we aim to discriminate between these two configurations. By including Herschel/SPIRE photometry, we extend the SED such that it now fully covers "},"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":"1405.1960","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2014-05-08T15:17:34Z","cross_cats_sorted":[],"title_canon_sha256":"c8820e1453ab5e27378def228b6ee6a0d8196bb5d3a873b1c424db0677ae2226","abstract_canon_sha256":"068ef4336c2476f2c3f7d729acba765c4c0540828bf6e22089c9a1d9268f4acb"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:43:35.725154Z","signature_b64":"EvOdqDAbSj2H+yhJH2PhXhIC4xwqtb+zNMTTII1xyLAV2FKJWh/Gz1Nd8acXASOnoY3CmTxo/eG+9jmowpT6AQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6b9232812a7950766a50986ba15a44099de34c0d5b66eb5afca115aef834bc68","last_reissued_at":"2026-05-18T02:43:35.724610Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:43:35.724610Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"An interferometric study of the post-AGB binary 89 Herculis. II Radiative transfer models of the circumbinary disk","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"C. Gielen, G. D. Mulders, H. Van Winckel, J. Menu, M. Hillen, M. Min, S. Regibo, T. Verhoelst, T. Wevers","submitted_at":"2014-05-08T15:17:34Z","abstract_excerpt":"The presence of disks and outflows is widespread among post-AGB binaries. In the first paper of this series, a surprisingly large fraction of optical light was found to be resolved in the 89 Her post-AGB system. The data showed this flux to arise from close to the central binary. Scattering off the inner rim of the circumbinary disk, or in a dusty outflow were suggested as two possible origins. With detailed dust radiative transfer models of the disk we aim to discriminate between these two configurations. By including Herschel/SPIRE photometry, we extend the SED such that it now fully covers "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1405.1960","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":"1405.1960","created_at":"2026-05-18T02:43:35.724690+00:00"},{"alias_kind":"arxiv_version","alias_value":"1405.1960v2","created_at":"2026-05-18T02:43:35.724690+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1405.1960","created_at":"2026-05-18T02:43:35.724690+00:00"},{"alias_kind":"pith_short_12","alias_value":"NOJDFAJKPFIH","created_at":"2026-05-18T12:28:41.024544+00:00"},{"alias_kind":"pith_short_16","alias_value":"NOJDFAJKPFIHM2SQ","created_at":"2026-05-18T12:28:41.024544+00:00"},{"alias_kind":"pith_short_8","alias_value":"NOJDFAJK","created_at":"2026-05-18T12:28:41.024544+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/NOJDFAJKPFIHM2SQTBV2CWSEBG","json":"https://pith.science/pith/NOJDFAJKPFIHM2SQTBV2CWSEBG.json","graph_json":"https://pith.science/api/pith-number/NOJDFAJKPFIHM2SQTBV2CWSEBG/graph.json","events_json":"https://pith.science/api/pith-number/NOJDFAJKPFIHM2SQTBV2CWSEBG/events.json","paper":"https://pith.science/paper/NOJDFAJK"},"agent_actions":{"view_html":"https://pith.science/pith/NOJDFAJKPFIHM2SQTBV2CWSEBG","download_json":"https://pith.science/pith/NOJDFAJKPFIHM2SQTBV2CWSEBG.json","view_paper":"https://pith.science/paper/NOJDFAJK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1405.1960&json=true","fetch_graph":"https://pith.science/api/pith-number/NOJDFAJKPFIHM2SQTBV2CWSEBG/graph.json","fetch_events":"https://pith.science/api/pith-number/NOJDFAJKPFIHM2SQTBV2CWSEBG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NOJDFAJKPFIHM2SQTBV2CWSEBG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NOJDFAJKPFIHM2SQTBV2CWSEBG/action/storage_attestation","attest_author":"https://pith.science/pith/NOJDFAJKPFIHM2SQTBV2CWSEBG/action/author_attestation","sign_citation":"https://pith.science/pith/NOJDFAJKPFIHM2SQTBV2CWSEBG/action/citation_signature","submit_replication":"https://pith.science/pith/NOJDFAJKPFIHM2SQTBV2CWSEBG/action/replication_record"}},"created_at":"2026-05-18T02:43:35.724690+00:00","updated_at":"2026-05-18T02:43:35.724690+00:00"}