{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2003:AI7YOA65QHRCSH2EHB5S4IATP2","short_pith_number":"pith:AI7YOA65","schema_version":"1.0","canonical_sha256":"023f8703dd81e2291f44387b2e20137e9b8a497cff99e7abd3de1d6616a1db6b","source":{"kind":"arxiv","id":"astro-ph/0310350","version":1},"attestation_state":"computed","paper":{"title":"Galaxy threshing and the origin of intracluster stellar objects","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"K. Bekki, M. D. Drinkwater, W. J. Couch, Y. Shioya","submitted_at":"2003-10-14T07:51:10Z","abstract_excerpt":"We numerically investigate dynamical evolution of non-nucleated dwarf elliptical/spiral galaxies (dE) and nucleated ones (dE,Ns) in clusters of galaxies in order to understand the origin of intracluster stellar objects, such as intracluster stars (ICSs), GCs (ICGCs), and ``ultra-compact dwarf'' (UCDs) recently discovered by all-object spectroscopic survey centred on the Fornax cluster of galaxies. We find that the outer stellar components of a nucleated dwarf are removed by the strong tidal field of the cluster, whereas the nucleus manages to survive as a result of its initially compact nature"},"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":"astro-ph/0310350","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2003-10-14T07:51:10Z","cross_cats_sorted":[],"title_canon_sha256":"8ca312d5e466ac3467bac29ae6c060a75d9185a755615255e6f1d6fabe9fbd34","abstract_canon_sha256":"4ab015cc41b9570feefe5e9c731ceebf246c6b80888c4d84149bba8011e0c523"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T14:13:04.935179Z","signature_b64":"2lwKZnzZrIbKJSHmHBpRf467TXeEIhmv90v0VE66qf+Ny7727qSX26OAAJ2z8E8QZbEbDHvDtOpwsclUJL0rDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"023f8703dd81e2291f44387b2e20137e9b8a497cff99e7abd3de1d6616a1db6b","last_reissued_at":"2026-07-04T14:13:04.934706Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T14:13:04.934706Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Galaxy threshing and the origin of intracluster stellar objects","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"K. Bekki, M. D. Drinkwater, W. J. Couch, Y. Shioya","submitted_at":"2003-10-14T07:51:10Z","abstract_excerpt":"We numerically investigate dynamical evolution of non-nucleated dwarf elliptical/spiral galaxies (dE) and nucleated ones (dE,Ns) in clusters of galaxies in order to understand the origin of intracluster stellar objects, such as intracluster stars (ICSs), GCs (ICGCs), and ``ultra-compact dwarf'' (UCDs) recently discovered by all-object spectroscopic survey centred on the Fornax cluster of galaxies. We find that the outer stellar components of a nucleated dwarf are removed by the strong tidal field of the cluster, whereas the nucleus manages to survive as a result of its initially compact nature"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0310350","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/astro-ph/0310350/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"astro-ph/0310350","created_at":"2026-07-04T14:13:04.934777+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0310350v1","created_at":"2026-07-04T14:13:04.934777+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0310350","created_at":"2026-07-04T14:13:04.934777+00:00"},{"alias_kind":"pith_short_12","alias_value":"AI7YOA65QHRC","created_at":"2026-07-04T14:13:04.934777+00:00"},{"alias_kind":"pith_short_16","alias_value":"AI7YOA65QHRCSH2E","created_at":"2026-07-04T14:13:04.934777+00:00"},{"alias_kind":"pith_short_8","alias_value":"AI7YOA65","created_at":"2026-07-04T14:13:04.934777+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2505.18251","citing_title":"Dynamical Evolutions in Globular Clusters and Dwarf Galaxies: Conduction Fluid Simulations","ref_index":9,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/AI7YOA65QHRCSH2EHB5S4IATP2","json":"https://pith.science/pith/AI7YOA65QHRCSH2EHB5S4IATP2.json","graph_json":"https://pith.science/api/pith-number/AI7YOA65QHRCSH2EHB5S4IATP2/graph.json","events_json":"https://pith.science/api/pith-number/AI7YOA65QHRCSH2EHB5S4IATP2/events.json","paper":"https://pith.science/paper/AI7YOA65"},"agent_actions":{"view_html":"https://pith.science/pith/AI7YOA65QHRCSH2EHB5S4IATP2","download_json":"https://pith.science/pith/AI7YOA65QHRCSH2EHB5S4IATP2.json","view_paper":"https://pith.science/paper/AI7YOA65","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0310350&json=true","fetch_graph":"https://pith.science/api/pith-number/AI7YOA65QHRCSH2EHB5S4IATP2/graph.json","fetch_events":"https://pith.science/api/pith-number/AI7YOA65QHRCSH2EHB5S4IATP2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/AI7YOA65QHRCSH2EHB5S4IATP2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/AI7YOA65QHRCSH2EHB5S4IATP2/action/storage_attestation","attest_author":"https://pith.science/pith/AI7YOA65QHRCSH2EHB5S4IATP2/action/author_attestation","sign_citation":"https://pith.science/pith/AI7YOA65QHRCSH2EHB5S4IATP2/action/citation_signature","submit_replication":"https://pith.science/pith/AI7YOA65QHRCSH2EHB5S4IATP2/action/replication_record"}},"created_at":"2026-07-04T14:13:04.934777+00:00","updated_at":"2026-07-04T14:13:04.934777+00:00"}