{"paper":{"title":"Burst-properties as a function of mass accretion rate in GX 3+1","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"1), 2), (2) Astronomical Institute, (3) Istituto Astrofisica Spaziale e Fisica Cosmica), A. Bazzano (3), E. Kuulkers (1, J. Heisse (2, J.J.M. in 't Zand (1, L.Natalucci (3), M. Cocchi (3), P.R. den Hartog (1, P. Ubertini (3) ((1) SRON - National Institute for Space Research, R.Cornelisse (1, The Netherlands, University of Utrecht","submitted_at":"2003-01-14T10:21:45Z","abstract_excerpt":"GX 3+1 is a low-mass X-ray binary that is persistently bright since its discovery in 1964. It was found to be an X-ray burster twenty years ago proving that the compact object in this system is a neutron star. The burst rate is so low that only 18 bursts were reported prior to 1996. The Wide Field Cameras on BeppoSAX have, through a dedicated monitoring program on the Galactic center region, increased the number of X-ray bursts from GX 3+1 by 61. Since GX 3+1 exhibits a slow (order of years) modulation in the persistent flux of about 50%, these observations opens up the unique possibility to s"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0301245","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"}