{"paper":{"title":"On the nature of eclipses in binary pulsar J0737-3039","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"CITA), Maxim Lyutikov (McGill University","submitted_at":"2004-03-03T16:40:33Z","abstract_excerpt":"We consider magnetohydrodynamical interaction between relativistic pulsar wind and static magnetosphere in binary pulsar system PSR J0737-3039. We construct semi-analytical model describing the form of the interface separating the two pulsars.\n An assumption of vacuum dipole spin down for Pulsar B leads to eclipse duration ten times longer than observed. We discuss possible Pulsar B torque modification and magnetic field estimates due to the interaction with\n Pulsar A wind.\n Unless the orbital inclination is $\\leq 86 ^\\circ$, the duration of eclipses is typically shorter than the one implied b"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0403076","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"}