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The Discovery of a Low-energy Excess in Cosmic-Ray Iron: Evidence of the Past Supernova Activity in the Local Bubble.

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第一作者： M J,Boschini

第一单位： INFN, Milano-Bicocca, Milano, Italy.;CINECA, Segrate, Milano, Italy.

作者： M J,Boschini ^[1] ; S,Della Torre ^[2] ; M,Gervasi ^[3] ; D,Grandi ^[3] ; G,Jóhannesson ^[4] ; G,La Vacca ^[3] ; N,Masi ^[5] ; I V,Moskalenko ^[6] ; S,Pensotti ^[3] ; T A,Porter ^[6] ; L,Quadrani ^[5] ; P G,Rancoita ^[2] ; D,Rozza ^[2] ; M,Tacconi ^[3]

作者单位： INFN, Milano-Bicocca, Milano, Italy.;CINECA, Segrate, Milano, Italy. ^[1] INFN, Milano-Bicocca, Milano, Italy. ^[2] INFN, Milano-Bicocca, Milano, Italy.;Physics Department, University of Milano-Bicocca, Milano, Italy. ^[3] Science Institute, University of Iceland, Dunhaga 3, IS-107 Reykjavik, Iceland.;NORDITA, Roslagstullsbacken 23, SE-106 91 Stockholm, Sweden. ^[4] INFN, Bologna, Italy.;Physics Department, University of Bologna, Bologna, Italy. ^[5] Hansen Experimental Physics Laboratory, Stanford University, Stanford, CA 94305, USA.;Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, Stanford, CA 94305, USA. ^[6]

关键词 Cosmic ray detectors (325)Cosmic ray sources (328)Galactic cosmic rays (567)Heliosphere (711)Interplanetary medium (825)Interstellar medium (847)

DOI 10.3847/1538-4357/abf11c

PMID 34646050

发布时间 2024-08-17

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