MULTIMESSENGER MODEL FOR THE STARBURST GALAXY M82

被引：61

作者：

de Cea del Pozo, Elsa ^{[1
]}

Torres, Diego F. ^{[1
]}

Rodriguez Marrero, Ana Y. ^{[1
]}

机构：

[1] CSIC, IEEC, Inst Ciencies Espai, Fac Ciencies, Barcelona 08193, Spain

来源：

ASTROPHYSICAL JOURNAL | 2009年 / 698卷 / 02期

关键词：

galaxies: individual (M82); galaxies: starburst; gamma rays: observations; gamma rays: theory; neutrinos; GAMMA-RAY EMISSION; HIGH-ENERGY EMISSION; HUBBLE-SPACE-TELESCOPE; COSMIC-RAY; STAR-FORMATION; SUPERNOVA-REMNANTS; MAGNETIC-FIELDS; HIGH-RESOLUTION; CONTINUUM OBSERVATIONS; SECONDARY ELECTRONS;

D O I：

10.1088/0004-637X/698/2/1054

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

In this paper, a consistent model of the multifrequency emission of the starburst galaxy M82, from radio to gamma-rays, is presented and discussed. Predictions for observations with Fermi, MAGIC II/VERITAS, and Cherenkov Telescope Array telescopes are made. The model is also used to self-consistently compute the (all flavors) emission of neutrinos resulting from this starburst galaxy. This can be used in considerations of diffuse contributions of such objects.

引用

页码：1054 / 1060

页数：7

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