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The short age estimated for the SNR qualifies SXP 1062 as the youngest known source in its class, ~ 10^4 yr. Here we discuss possible evolutionary scenarios for SXP 1062 in the attempt to reconcile its long spin period, P=1062 s, and short age. Our results indicate that SXP 1062 may host a neutron star born with a large initial magnetic field, typically in excess of ~ 10^14 G, which then decayed to ~ 10^13 G."},"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":"1206.3487","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2012-06-15T14:46:29Z","cross_cats_sorted":[],"title_canon_sha256":"ed06283838ab0e682a731d9472b3c8910f5934e4ca2e3f759556242c2ee4f688","abstract_canon_sha256":"b0e316971837f6373acf86ec5e214d25ae124d9df7e244a8be7f8bea72bf97f9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:35:12.679576Z","signature_b64":"DgxPoECVSm5vl+eGXUrZ/yX8llSe4iLc7gSTZCP7DYitIe3DH/xz+lpLMuaGHzsko3mclu9CDW7owhICz/7oDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"15beeb24852622b0cd8adfc707f22760e9f299ba8cb5d66c724eb79db4ca74a2","last_reissued_at":"2026-05-18T01:35:12.678698Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:35:12.678698Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"SXP 1062: an Evolved Magnetar in a BeXB ?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Italy, MSSL-UCL, R. 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