ULTRA-HIGH RESOLUTION GAMMA-RAY RESONANCE IN ZINC-67

被引:16
|
作者
NAGLE, DE
CRAIG, PP
KELLER, WE
机构
关键词
D O I
10.1038/186707a0
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
引用
收藏
页码:707 / 708
页数:2
相关论文
共 50 条
  • [41] Gamma-ray bursts, ultra-high-energy cosmic rays, and cosmic gamma-ray background
    Totani, T
    ASTROPARTICLE PHYSICS, 1999, 11 (04) : 451 - 455
  • [42] TeV gamma-ray emission from gamma-ray bursts and ultra high energy cosmic rays
    Totani, T
    ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES, 2000, 142 (03): : 443 - 445
  • [43] Ultra-long gamma-ray bursts and ultra-soft gamma-ray bursts
    Huang Yan
    Luo Qi
    Zhang BinBin
    Xiong ShaoLin
    SCIENTIA SINICA-PHYSICA MECHANICA & ASTRONOMICA, 2020, 50 (12)
  • [44] Diffusion of ultra-high energy protons in galaxy clusters and secondary X- and gamma-ray emissions
    Rordorf, C
    Grasso, D
    Dolag, K
    ASTROPARTICLE PHYSICS, 2004, 22 (02) : 167 - 181
  • [45] Ultra-high Energy Cosmic Rays and Neutrinos from Gamma-Ray Bursts, Hypernovae and Galactic Shocks
    Meszaros, P.
    NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS, 2014, 256 : 241 - 251
  • [46] Upper limits on ultra-high energy neutrino fluxes from cosmic and gamma-ray data.
    Semikoz, DV
    NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS, 2003, 118 : 519 - 519
  • [47] Prospects for high angular resolution in gamma-ray astronomy
    Skinner, GK
    GALAXIES AND THEIR CONSTITUENTS AT THE HIGHEST ANGULAR RESOLUTIONS, 2001, (205): : 463 - 468
  • [48] Instrument concepts for high resolution gamma-ray spectroscopy
    Jean, P
    Naya, JE
    Olive, JF
    vonBallmoos, P
    ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES, 1996, 120 (04): : C673 - C676
  • [49] CALIBRATION OF THE HIGH AND LOW RESOLUTION GAMMA-RAY SPECTROMETERS
    Luca, Aurelian
    Neacsu, Beatris
    Antohe, Andrei
    Sahagia, Maria
    ROMANIAN REPORTS IN PHYSICS, 2012, 64 (04) : 968 - 976
  • [50] ASGAT - A HIGH-RESOLUTION GAMMA-RAY TELESCOPE
    BASIUK, V
    COSMIC GAMMA RAYS, NEUTRINOS, AND RELATED ASTROPHYSICS, 1989, 270 : 443 - 448