{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:DIYVE7INHD7JRYHIJUFIXAPVTR","short_pith_number":"pith:DIYVE7IN","schema_version":"1.0","canonical_sha256":"1a31527d0d38fe98e0e84d0a8b81f59c5e6948873e3fcc8b596e6a5dd319b96a","source":{"kind":"arxiv","id":"1710.03311","version":2},"attestation_state":"computed","paper":{"title":"A molecular-line study of the interstellar bullet engine IRAS 05506+2414","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.GA","authors_text":"Carmen Sanchez Contreras, Chin-Fei Lee, Mark Claussen, Mark R. Morris, Nimesh Patel, Raghvendra Sahai","submitted_at":"2017-10-09T20:55:57Z","abstract_excerpt":"We present interferometric and single-dish molecular line observations of the interstellar bullet-outflow source IRAS 05506+2414, whose wide-angle bullet spray is similar to the Orion BN/KL explosive outflow and likely arises from an entirely different mechanism than the classical accretion-disk-driven bipolar flows in young stellar objects. The bullet-outflow source is associated with a large pseudo-disk and three molecular outflows -- a high-velocity outflow (HVO), a medium-velocity outflow (MVO), and a slow, extended outflow (SEO). The size (mass) of the pseudo-disk is 10,350 AU x 6,400 AU "},"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":"1710.03311","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-10-09T20:55:57Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"f03851776c4a200ec7bc030c42b52421dc13d52416020242c3b2e4d64888e2e5","abstract_canon_sha256":"a849ade2c16a4e15ebd4a250e379ded565e0ede7ebf7ea9eff904022fb32cdf4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:28:13.639350Z","signature_b64":"s09sqsBfQlVSyAN/rqfGP7cSIfNrT5WNFQAo6vVBxwZY/tqZZbOxOuo7eLFJzdNT1ujiEWPennoiEezNZgmdCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1a31527d0d38fe98e0e84d0a8b81f59c5e6948873e3fcc8b596e6a5dd319b96a","last_reissued_at":"2026-05-18T00:28:13.638608Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:28:13.638608Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A molecular-line study of the interstellar bullet engine IRAS 05506+2414","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.GA","authors_text":"Carmen Sanchez Contreras, Chin-Fei Lee, Mark Claussen, Mark R. Morris, Nimesh Patel, Raghvendra Sahai","submitted_at":"2017-10-09T20:55:57Z","abstract_excerpt":"We present interferometric and single-dish molecular line observations of the interstellar bullet-outflow source IRAS 05506+2414, whose wide-angle bullet spray is similar to the Orion BN/KL explosive outflow and likely arises from an entirely different mechanism than the classical accretion-disk-driven bipolar flows in young stellar objects. The bullet-outflow source is associated with a large pseudo-disk and three molecular outflows -- a high-velocity outflow (HVO), a medium-velocity outflow (MVO), and a slow, extended outflow (SEO). The size (mass) of the pseudo-disk is 10,350 AU x 6,400 AU "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1710.03311","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":"1710.03311","created_at":"2026-05-18T00:28:13.638724+00:00"},{"alias_kind":"arxiv_version","alias_value":"1710.03311v2","created_at":"2026-05-18T00:28:13.638724+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1710.03311","created_at":"2026-05-18T00:28:13.638724+00:00"},{"alias_kind":"pith_short_12","alias_value":"DIYVE7INHD7J","created_at":"2026-05-18T12:31:10.602751+00:00"},{"alias_kind":"pith_short_16","alias_value":"DIYVE7INHD7JRYHI","created_at":"2026-05-18T12:31:10.602751+00:00"},{"alias_kind":"pith_short_8","alias_value":"DIYVE7IN","created_at":"2026-05-18T12:31:10.602751+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/DIYVE7INHD7JRYHIJUFIXAPVTR","json":"https://pith.science/pith/DIYVE7INHD7JRYHIJUFIXAPVTR.json","graph_json":"https://pith.science/api/pith-number/DIYVE7INHD7JRYHIJUFIXAPVTR/graph.json","events_json":"https://pith.science/api/pith-number/DIYVE7INHD7JRYHIJUFIXAPVTR/events.json","paper":"https://pith.science/paper/DIYVE7IN"},"agent_actions":{"view_html":"https://pith.science/pith/DIYVE7INHD7JRYHIJUFIXAPVTR","download_json":"https://pith.science/pith/DIYVE7INHD7JRYHIJUFIXAPVTR.json","view_paper":"https://pith.science/paper/DIYVE7IN","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1710.03311&json=true","fetch_graph":"https://pith.science/api/pith-number/DIYVE7INHD7JRYHIJUFIXAPVTR/graph.json","fetch_events":"https://pith.science/api/pith-number/DIYVE7INHD7JRYHIJUFIXAPVTR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DIYVE7INHD7JRYHIJUFIXAPVTR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DIYVE7INHD7JRYHIJUFIXAPVTR/action/storage_attestation","attest_author":"https://pith.science/pith/DIYVE7INHD7JRYHIJUFIXAPVTR/action/author_attestation","sign_citation":"https://pith.science/pith/DIYVE7INHD7JRYHIJUFIXAPVTR/action/citation_signature","submit_replication":"https://pith.science/pith/DIYVE7INHD7JRYHIJUFIXAPVTR/action/replication_record"}},"created_at":"2026-05-18T00:28:13.638724+00:00","updated_at":"2026-05-18T00:28:13.638724+00:00"}