{"paper":{"title":"X-ray study of extended emission around M86 observed with Suzaku","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Hiromasa Ito, Keigo Tanaka, Misato Kotake, Ryuichi Fujimoto, Ukyo Hishi, Yu Kai, Yuya Kinoshita","submitted_at":"2017-02-20T08:04:53Z","abstract_excerpt":"We analyzed the Suzaku data of M86 and its adjacent regions to study the extended emission around it. The M86 core, the plume, and the tail extending toward the northwest were clearly detected, as well as the extended halo around them. From the position angle $\\sim45\\deg$ to $\\sim275\\deg$, the surface brightness distribution of the core and the extended halo was represented relatively well with a single $\\beta$-model of $\\beta\\sim0.5$ up to 15'-20'. The X-ray spectra of the core was represented with a two-temperature model of $kT\\sim 0.9$ keV and $\\sim0.6$ keV. The temperatures of the core and"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1702.05887","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"}