{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:TZ5QMZDAEUH5KC5AD2QKESSPMU","short_pith_number":"pith:TZ5QMZDA","schema_version":"1.0","canonical_sha256":"9e7b066460250fd50ba01ea0a24a4f6509e7ed7a81b840ad546bc96b4d829d12","source":{"kind":"arxiv","id":"2312.03272","version":2},"attestation_state":"computed","paper":{"title":"Multiple shells driven by disk winds: ALMA observations in the HH 30 outflow","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.SR","authors_text":"Chin-Fei Lee, Fabien Louvet, J. A. L\\'opez-V\\'azquez, Luis A. Zapata, M. Fern\\'andez-L\\'opez, O. Guerra-Alvarado","submitted_at":"2023-12-06T03:58:25Z","abstract_excerpt":"We present archive Atacama Large Millimeter/Submillimeter Array (ALMA) Band 6 observations of the $^{13}$CO (J=2-1) and $^{12}$CO (J=2-1) molecular line emission of the protostellar system associated with HH 30. The $^{13}$CO molecular line shows the accretion disk while the molecular outflow is traced by the emission of the $^{12}$CO molecular line. We estimated a dynamical mass for the central object of $0.45\\pm0.14$ M$_\\odot$, and a mass for the molecular outflow of $1.83\\pm0.19\\times10^{-4}$ M$_\\odot$. The molecular outflow presents an internal cavity as well as multiple outflowing shell s"},"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":"2312.03272","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2023-12-06T03:58:25Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"049b3c11765a81d90fe846a46c16f8a89405f4319b72b0743c2036ba9b3b86e7","abstract_canon_sha256":"89acf0e6d5109967f2c5eaef6aca03af157d24b2b47fa792679df7da29b95947"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:21:47.213866Z","signature_b64":"z3L97OyfsjmECNbDQvH1RgCsTt70Ujp0uGPg/Ag1x9bjH932Uw7pGOyKc0zYeskyB3/9jpRAHAaAZloihe/1BA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9e7b066460250fd50ba01ea0a24a4f6509e7ed7a81b840ad546bc96b4d829d12","last_reissued_at":"2026-07-05T07:21:47.213441Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:21:47.213441Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Multiple shells driven by disk winds: ALMA observations in the HH 30 outflow","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.SR","authors_text":"Chin-Fei Lee, Fabien Louvet, J. A. L\\'opez-V\\'azquez, Luis A. Zapata, M. Fern\\'andez-L\\'opez, O. Guerra-Alvarado","submitted_at":"2023-12-06T03:58:25Z","abstract_excerpt":"We present archive Atacama Large Millimeter/Submillimeter Array (ALMA) Band 6 observations of the $^{13}$CO (J=2-1) and $^{12}$CO (J=2-1) molecular line emission of the protostellar system associated with HH 30. The $^{13}$CO molecular line shows the accretion disk while the molecular outflow is traced by the emission of the $^{12}$CO molecular line. We estimated a dynamical mass for the central object of $0.45\\pm0.14$ M$_\\odot$, and a mass for the molecular outflow of $1.83\\pm0.19\\times10^{-4}$ M$_\\odot$. The molecular outflow presents an internal cavity as well as multiple outflowing shell s"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2312.03272","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2312.03272/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":"2312.03272","created_at":"2026-07-05T07:21:47.213495+00:00"},{"alias_kind":"arxiv_version","alias_value":"2312.03272v2","created_at":"2026-07-05T07:21:47.213495+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2312.03272","created_at":"2026-07-05T07:21:47.213495+00:00"},{"alias_kind":"pith_short_12","alias_value":"TZ5QMZDAEUH5","created_at":"2026-07-05T07:21:47.213495+00:00"},{"alias_kind":"pith_short_16","alias_value":"TZ5QMZDAEUH5KC5A","created_at":"2026-07-05T07:21:47.213495+00:00"},{"alias_kind":"pith_short_8","alias_value":"TZ5QMZDA","created_at":"2026-07-05T07:21:47.213495+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/TZ5QMZDAEUH5KC5AD2QKESSPMU","json":"https://pith.science/pith/TZ5QMZDAEUH5KC5AD2QKESSPMU.json","graph_json":"https://pith.science/api/pith-number/TZ5QMZDAEUH5KC5AD2QKESSPMU/graph.json","events_json":"https://pith.science/api/pith-number/TZ5QMZDAEUH5KC5AD2QKESSPMU/events.json","paper":"https://pith.science/paper/TZ5QMZDA"},"agent_actions":{"view_html":"https://pith.science/pith/TZ5QMZDAEUH5KC5AD2QKESSPMU","download_json":"https://pith.science/pith/TZ5QMZDAEUH5KC5AD2QKESSPMU.json","view_paper":"https://pith.science/paper/TZ5QMZDA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2312.03272&json=true","fetch_graph":"https://pith.science/api/pith-number/TZ5QMZDAEUH5KC5AD2QKESSPMU/graph.json","fetch_events":"https://pith.science/api/pith-number/TZ5QMZDAEUH5KC5AD2QKESSPMU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TZ5QMZDAEUH5KC5AD2QKESSPMU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TZ5QMZDAEUH5KC5AD2QKESSPMU/action/storage_attestation","attest_author":"https://pith.science/pith/TZ5QMZDAEUH5KC5AD2QKESSPMU/action/author_attestation","sign_citation":"https://pith.science/pith/TZ5QMZDAEUH5KC5AD2QKESSPMU/action/citation_signature","submit_replication":"https://pith.science/pith/TZ5QMZDAEUH5KC5AD2QKESSPMU/action/replication_record"}},"created_at":"2026-07-05T07:21:47.213495+00:00","updated_at":"2026-07-05T07:21:47.213495+00:00"}