Supernova Remnants with Fermi Large Area Telescope

被引：0

作者：

Caragiulo, M. ^{[1
,2
]}

Di Venere, L. ^{[1
,2
]}

机构：

[1] Dipartimento Interateneo Fis Michelangelo Merlin, Via Amendola 173, I-70126 Bari, Italy

[2] Ist Nazl Fis Nucl INFN, Sez INFN Bari, Via Orabona 4, I-70126 Bari, Italy

来源：

RICAP16, 6TH ROMA INTERNATIONAL CONFERENCE ON ASTROPARTICLE PHYSICS | 2017年 / 136卷

基金：

瑞典研究理事会;

关键词：

RX J1713.7-3946; ACCELERATION;

D O I：

10.1051/epjconf/201713603012

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The Large Area Telescope (LAT), on-board the Fermi satellite, proved to be, after 8 years of data taking, an excellent instrument to detect and observe Supernova Remnants (SNRs) in a range of energies running from few hundred MeV up to few hundred GeV. It provides essential information on physical processes that occur at the source, involving both accelerated leptons and hadrons, in order to understand the mechanisms responsible for the primary Cosmic Ray (CR) acceleration. We show the latest results in the observation of Galactic SNRs by Fermi-LAT.

引用

页数：7

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