Detection of the characteristic pion-decay signature in supernova remnants.
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An embryo of protocells: The capsule of graphene with selective ion channelsOrganic Matter Responses to Radiation under Lunar Conditions.Chemical Imaging of Xylem by Raman Microspectroscopy.A rapid cosmic-ray increase in BC 3372-3371 from ancient buried tree rings in China.Direct detection of a break in the teraelectronvolt cosmic-ray spectrum of electrons and positrons.Electron Surfing and Drift Accelerations in a Weibel-Dominated High-Mach-Number Shock.Supernova Origin of Cosmic Rays from a γ-Ray Signal in the Constellation III Region of the Large Magellanic Cloud.Generation and Evolution of High-Mach-Number Laser-Driven Magnetized Collisionless Shocks in the Laboratory.Filamentation instability of counterstreaming laser-driven plasmas.Latest results from VERITAS: Gamma 2016Limit on the ultrahigh-energy neutrino flux from lunar observations with the Parkes radio telescopeSupernova Remnants Interacting with Molecular Clouds: X-Ray and Gamma-Ray SignaturesRecent results in nuclear astrophysicsA cut-off in the TeV gamma-ray spectrum of the SNR Cassiopeia ASearch for neutrino-induced particle showers with IceCube-40Toward a comprehensive global electric circuit model: Atmospheric conductivity and its variability in CESM1(WACCM) model simulationsCollisionless electrostatic shock generation using high-energy laser systemsSupernova remnant W44: a case of cosmic-ray reaccelerationRecent Results in Cosmic Ray Physics and Their InterpretationThe origin of galactic cosmic raysSupernova remnants in the Local Group – I. A model for the radio luminosity function and visibility times of supernova remnantsThe e-ASTROGAM missionH.E.S.S. detection of TeV emission from the interaction region between the supernova remnant G349.7+0.2 and a molecular cloudImaging of SNR IC443 and W44 with the Sardinia Radio Telescope at 1.5 and 7 GHzHigh-resolution spectral imaging of SNR W44 and IC443 at 22 GHz with the Sardinia Radio TelescopeMultimolecule ALMA observations toward the Seyfert 1 galaxy NGC 1097Cosmic Rays Report from the Structure of SpaceCosmic rays originate from supernova shockwaves
P2860
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P2860
Detection of the characteristic pion-decay signature in supernova remnants.
description
2013 nî lūn-bûn
@nan
2013 թուականի Փետրուարին հրատարակուած գիտական յօդուած
@hyw
2013 թվականի փետրվարին հրատարակված գիտական հոդված
@hy
2013年の論文
@ja
2013年論文
@yue
2013年論文
@zh-hant
2013年論文
@zh-hk
2013年論文
@zh-mo
2013年論文
@zh-tw
2013年论文
@wuu
name
Detection of the characteristic pion-decay signature in supernova remnants.
@ast
Detection of the characteristic pion-decay signature in supernova remnants.
@en
Detection of the characteristic pion-decay signature in supernova remnants.
@nl
type
label
Detection of the characteristic pion-decay signature in supernova remnants.
@ast
Detection of the characteristic pion-decay signature in supernova remnants.
@en
Detection of the characteristic pion-decay signature in supernova remnants.
@nl
prefLabel
Detection of the characteristic pion-decay signature in supernova remnants.
@ast
Detection of the characteristic pion-decay signature in supernova remnants.
@en
Detection of the characteristic pion-decay signature in supernova remnants.
@nl
P2093
P50
P356
P1433
P1476
Detection of the characteristic pion-decay signature in supernova remnants.
@en
P2093
A A Moiseev
A Allafort
A Chekhtman
A Drlica-Wagner
A Franckowiak
A K Harding
A N Cillis
A S Johnson
P304
P356
10.1126/SCIENCE.1231160
P407
P50
P577
2013-02-01T00:00:00Z
P5875
P698
P818
P819
2013Sci...339..807A