{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2017:U3TKPO4O2YW27KFK4GPDB4KA5N","short_pith_number":"pith:U3TKPO4O","canonical_record":{"source":{"id":"1708.00473","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2017-08-01T18:48:37Z","cross_cats_sorted":[],"title_canon_sha256":"a58c6df18d489bd95b71ce78b77b84c1dd56be609900c42a5ad0228c48caf036","abstract_canon_sha256":"73e0b2491606e927befa7f7f97ca8d579182ed3d087e78a20d024a94d801d336"},"schema_version":"1.0"},"canonical_sha256":"a6e6a7bb8ed62dafa8aae19e30f140eb6e2b7e5cc75a7fc8f16f41bf758e867d","source":{"kind":"arxiv","id":"1708.00473","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1708.00473","created_at":"2026-05-18T00:36:27Z"},{"alias_kind":"arxiv_version","alias_value":"1708.00473v1","created_at":"2026-05-18T00:36:27Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1708.00473","created_at":"2026-05-18T00:36:27Z"},{"alias_kind":"pith_short_12","alias_value":"U3TKPO4O2YW2","created_at":"2026-05-18T12:31:46Z"},{"alias_kind":"pith_short_16","alias_value":"U3TKPO4O2YW27KFK","created_at":"2026-05-18T12:31:46Z"},{"alias_kind":"pith_short_8","alias_value":"U3TKPO4O","created_at":"2026-05-18T12:31:46Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2017:U3TKPO4O2YW27KFK4GPDB4KA5N","target":"record","payload":{"canonical_record":{"source":{"id":"1708.00473","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2017-08-01T18:48:37Z","cross_cats_sorted":[],"title_canon_sha256":"a58c6df18d489bd95b71ce78b77b84c1dd56be609900c42a5ad0228c48caf036","abstract_canon_sha256":"73e0b2491606e927befa7f7f97ca8d579182ed3d087e78a20d024a94d801d336"},"schema_version":"1.0"},"canonical_sha256":"a6e6a7bb8ed62dafa8aae19e30f140eb6e2b7e5cc75a7fc8f16f41bf758e867d","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:36:27.960130Z","signature_b64":"kn5Spn5VLN9SiNDD9HEN0+SXTPkte1Ogty2Ltx+UKqRNX0EDFwo/6wWKlmJNgHcObyBuUWhHb0cXsFShh98eDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a6e6a7bb8ed62dafa8aae19e30f140eb6e2b7e5cc75a7fc8f16f41bf758e867d","last_reissued_at":"2026-05-18T00:36:27.959348Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:36:27.959348Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1708.00473","source_version":1,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T00:36:27Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"wym4IRc7Rs2YfdouqhsimkCCMrbgQegOJ0ixbPVVMBU3Q6XMAkiEeJ9Mg54qp0imIERhtEapuoYOXhP9LKL8DQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-26T15:58:18.002567Z"},"content_sha256":"873df8e3849092ed44c908421c89eaf29a3e0683107cd66710759248690c3607","schema_version":"1.0","event_id":"sha256:873df8e3849092ed44c908421c89eaf29a3e0683107cd66710759248690c3607"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2017:U3TKPO4O2YW27KFK4GPDB4KA5N","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"$\\Omega$-Slow Solutions and Be Star Disks","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Granada, A. Jim\\'enez, C. E. Jones, I. Araya, J. Silaj, L. Cidale, M. Cur\\'e","submitted_at":"2017-08-01T18:48:37Z","abstract_excerpt":"As the disk formation mechanism(s) in Be stars is(are) as yet unknown, we investigate the role of rapidly rotating radiation-driven winds in this process. We implemented the effects of high stellar rotation on m-CAK models accounting for: the shape of the star, the oblate finite disk correction factor, and gravity darkening. For a fast rotating star, we obtain a two-component wind model, i.e., a fast, thin wind in the polar latitudes and an $\\Omega$-slow, dense wind in the equatorial regions. We use the equatorial mass densities to explore H$\\alpha$ emission profiles for the following scenario"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1708.00473","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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T00:36:27Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"IPcT8+iVENKw6dqvkDbnfCeXj7XeP1urfV5ofx/Gx6YPpx9WnE0l6mlxmPqcCq9N2JWLRWgxrxcPydmJ+DptCA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-26T15:58:18.003211Z"},"content_sha256":"fce32b02ec71652cf2d8aec1f7bd0c11124568602a7a9acb1632dd8a5f5646f0","schema_version":"1.0","event_id":"sha256:fce32b02ec71652cf2d8aec1f7bd0c11124568602a7a9acb1632dd8a5f5646f0"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/U3TKPO4O2YW27KFK4GPDB4KA5N/bundle.json","state_url":"https://pith.science/pith/U3TKPO4O2YW27KFK4GPDB4KA5N/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/U3TKPO4O2YW27KFK4GPDB4KA5N/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-05-26T15:58:18Z","links":{"resolver":"https://pith.science/pith/U3TKPO4O2YW27KFK4GPDB4KA5N","bundle":"https://pith.science/pith/U3TKPO4O2YW27KFK4GPDB4KA5N/bundle.json","state":"https://pith.science/pith/U3TKPO4O2YW27KFK4GPDB4KA5N/state.json","well_known_bundle":"https://pith.science/.well-known/pith/U3TKPO4O2YW27KFK4GPDB4KA5N/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2017:U3TKPO4O2YW27KFK4GPDB4KA5N","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"73e0b2491606e927befa7f7f97ca8d579182ed3d087e78a20d024a94d801d336","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2017-08-01T18:48:37Z","title_canon_sha256":"a58c6df18d489bd95b71ce78b77b84c1dd56be609900c42a5ad0228c48caf036"},"schema_version":"1.0","source":{"id":"1708.00473","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1708.00473","created_at":"2026-05-18T00:36:27Z"},{"alias_kind":"arxiv_version","alias_value":"1708.00473v1","created_at":"2026-05-18T00:36:27Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1708.00473","created_at":"2026-05-18T00:36:27Z"},{"alias_kind":"pith_short_12","alias_value":"U3TKPO4O2YW2","created_at":"2026-05-18T12:31:46Z"},{"alias_kind":"pith_short_16","alias_value":"U3TKPO4O2YW27KFK","created_at":"2026-05-18T12:31:46Z"},{"alias_kind":"pith_short_8","alias_value":"U3TKPO4O","created_at":"2026-05-18T12:31:46Z"}],"graph_snapshots":[{"event_id":"sha256:fce32b02ec71652cf2d8aec1f7bd0c11124568602a7a9acb1632dd8a5f5646f0","target":"graph","created_at":"2026-05-18T00:36:27Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"paper":{"abstract_excerpt":"As the disk formation mechanism(s) in Be stars is(are) as yet unknown, we investigate the role of rapidly rotating radiation-driven winds in this process. We implemented the effects of high stellar rotation on m-CAK models accounting for: the shape of the star, the oblate finite disk correction factor, and gravity darkening. For a fast rotating star, we obtain a two-component wind model, i.e., a fast, thin wind in the polar latitudes and an $\\Omega$-slow, dense wind in the equatorial regions. We use the equatorial mass densities to explore H$\\alpha$ emission profiles for the following scenario","authors_text":"A. Granada, A. Jim\\'enez, C. E. Jones, I. Araya, J. Silaj, L. Cidale, M. Cur\\'e","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2017-08-01T18:48:37Z","title":"$\\Omega$-Slow Solutions and Be Star Disks"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1708.00473","kind":"arxiv","version":1},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:873df8e3849092ed44c908421c89eaf29a3e0683107cd66710759248690c3607","target":"record","created_at":"2026-05-18T00:36:27Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"73e0b2491606e927befa7f7f97ca8d579182ed3d087e78a20d024a94d801d336","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2017-08-01T18:48:37Z","title_canon_sha256":"a58c6df18d489bd95b71ce78b77b84c1dd56be609900c42a5ad0228c48caf036"},"schema_version":"1.0","source":{"id":"1708.00473","kind":"arxiv","version":1}},"canonical_sha256":"a6e6a7bb8ed62dafa8aae19e30f140eb6e2b7e5cc75a7fc8f16f41bf758e867d","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"a6e6a7bb8ed62dafa8aae19e30f140eb6e2b7e5cc75a7fc8f16f41bf758e867d","first_computed_at":"2026-05-18T00:36:27.959348Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T00:36:27.959348Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"kn5Spn5VLN9SiNDD9HEN0+SXTPkte1Ogty2Ltx+UKqRNX0EDFwo/6wWKlmJNgHcObyBuUWhHb0cXsFShh98eDQ==","signature_status":"signed_v1","signed_at":"2026-05-18T00:36:27.960130Z","signed_message":"canonical_sha256_bytes"},"source_id":"1708.00473","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:873df8e3849092ed44c908421c89eaf29a3e0683107cd66710759248690c3607","sha256:fce32b02ec71652cf2d8aec1f7bd0c11124568602a7a9acb1632dd8a5f5646f0"],"state_sha256":"c712515409e76f47e649fe2275bc30b306e9035a1185475a91ae0e96812bcfb5"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"PbvKsYRIA07spSswg+YMwvLN3LK3xCGpwZ1ksqXhCM7nWdt/Mxr/8Hf6uEe149DNFPEr1seQ99Y+GVxueDSeAA==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-26T15:58:18.006901Z","bundle_sha256":"622736dc05cdca18e808fda45aec4dc8d79016603065376ff6babeba600534a6"}}