机译:从NGC 253的磁力开始的巨型光晕的快速谱变化
Univ Space & Res Assoc Huntsville AL 35805 USA;
Univ Alabama Ctr Space Plasma & Aeronom Res Huntsville AL 35899 USA;
Rice Univ Dept Phys & Astron Houston TX 77005 USA;
Univ Alabama Ctr Space Plasma & Aeronom Res Huntsville AL 35899 USA|Univ Alabama Dept Space Sci Huntsville AL 35899 USA;
George Washington Univ Dept Phys Washington DC 20052 USA|George Washington Univ Astron Phys & Stat Inst Sci APSIS Washington DC USA;
Univ Politecn Bari Dipartimento Fis M Merlin Bari Italy|Ist Nazl Fis Nucl Bari Italy;
George Washington Univ Dept Phys Washington DC 20052 USA|George Washington Univ Astron Phys & Stat Inst Sci APSIS Washington DC USA;
George Washington Univ Dept Phys Washington DC 20052 USA|George Washington Univ Astron Phys & Stat Inst Sci APSIS Washington DC USA;
Penn State Univ Dept Phys 104 Davey Lab University Pk PA 16802 USA;
Univ Washington Dept Astron Ctr Data Intens Res Astron & Cosmol DIRAC Seattle WA 98195 USA;
Univ Toronto Dept Astron & Astrophys Toronto ON Canada;
Univ Alabama Ctr Space Plasma & Aeronom Res Huntsville AL 35899 USA|Univ Alabama Dept Space Sci Huntsville AL 35899 USA;
Sabanci Univ Fac Engn & Nat Sci Istanbul Turkey;
George Washington Univ Dept Phys Washington DC 20052 USA|George Washington Univ Astron Phys & Stat Inst Sci APSIS Washington DC USA;
Penn State Univ Dept Astron & Astrophys 525 Davey Lab University Pk PA 16802 USA;
NASA Astrophys Branch ST12 Marshall Space Flight Ctr MSFC Huntsville AL USA;
Natl Radio Astron Observ Socorro NM 87801 USA;
George Washington Univ Dept Phys Washington DC 20052 USA|George Washington Univ Astron Phys & Stat Inst Sci APSIS Washington DC USA|NASA Goddard Space Flight Ctr GSFC Greenbelt MD USA;
Univ Alabama Ctr Space Plasma & Aeronom Res Huntsville AL 35899 USA|Univ Alabama Dept Space Sci Huntsville AL 35899 USA;
NASA Astrophys Branch ST12 Marshall Space Flight Ctr MSFC Huntsville AL USA;
Louisiana State Univ Dept Phys & Astron Baton Rouge LA 70803 USA;
机译:一个明亮的γ射线火炬被解释为NGC253的巨型磁力耀斑
机译:巨大耀斑后,CHANDR以SGR 1806-20的第一眼:显着的光谱软化和快速通量衰减
机译:巨大耀斑后,CHANDR以SGR 1806-20的第一眼:显着的光谱软化和快速通量衰减
机译:丙灭核的化学复杂性:ARP 220,NGC 253和NGC 4945用顶尖望远镜调查
机译:Z-Spec:用于毫米波天体物理学的宽带光谱仪-仪器的开发以及对附近恒星形成星系NGC 253的分子线测量的结果
机译:巨大的蝴蝶蛾Paysandisia执政官拥有丰富光谱的并置眼睛具有独特的光依赖性感光器动力学
机译:在巨型耀斑之后,Chandra首次亮相1806-20 sGR: 显着的光谱软化和快速的通量衰减