机译:在两个中子恒星的合并之后,富含镧系元素的千克诺瓦的出现
University of Leicester Department of Physics &
Astronomy and Leicester Institute of Space &
Earth Observation University Road Leicester LE1 7RH UK;
Department of Physics University of Warwick Coventry CV4 7AL UK;
Institute of Astronomy University of Cambridge Madingley Road Cambridge CB3 0HA UK;
Computational Methods Group (CCS-2) Los Alamos National Laboratory P.O. Box 1663 Los Alamos NM 87545 USA;
Birmingham Institute for Gravitational Wave Astronomy and School of Physics and Astronomy University of Birmingham Birmingham B15 2TT UK;
The Oskar Klein Centre Department of Astronomy AlbaNova Stockholm University SE-106 91 Stockholm Sweden;
Dark Cosmology Centre Niels Bohr Institute University of Copenhagen Juliane Maries Vej 30 DK-2100 Copenhagen ? Denmark;
INAF Osservatorio Astronomico di Brera Via E. Bianchi 46 I-23807 Merate (LC) Italy;
Space Telescope Science Institute 3700 San Martin Drive Baltimore MD 21218 USA;
Computational Methods Group (CCS-2) Los Alamos National Laboratory P.O. Box 1663 Los Alamos NM 87545 USA;
Space Telescope Science Institute 3700 San Martin Drive Baltimore MD 21218 USA;
Dark Cosmology Centre Niels Bohr Institute University of Copenhagen Juliane Maries Vej 30 DK-2100 Copenhagen ? Denmark;
University of Leicester Department of Physics &
Astronomy and Leicester Institute of Space &
Earth Observation University Road Leicester LE1 7RH UK;
Department of Physics University of Warwick Coventry CV4 7AL UK;
Computational Methods Group (CCS-2) Los Alamos National Laboratory P.O. Box 1663 Los Alamos NM 87545 USA;
Instituto de Astrofísica de Andalucía (IAA-CSIC) Glorieta de la Astronomía s/n 18008 Granada Spain;
Astrophysics Research Institute Liverpool John Moores University Liverpool Science Park IC2 146 Brownlow Hill Liverpool L3 5RF UK;
INAF Osservatorio Astronomico di Brera Via E. Bianchi 46 I-23807 Merate (LC) Italy;
Space Science Data Center ASI Via del Politecnico s.n.c. I-00133 Roma Italy;
Dark Cosmology Centre Niels Bohr Institute University of Copenhagen Juliane Maries Vej 30 DK-2100 Copenhagen ? Denmark;
University of Leicester Department of Physics &
Astronomy and Leicester Institute of Space &
Earth Observation University Road Leicester LE1 7RH UK;
Computational Methods Group (CCS-2) Los Alamos National Laboratory P.O. Box 1663 Los Alamos NM 87545 USA;
School of Physics and Astronomy Cardiff University Cardiff UK;
SUPA School of Physics &
Astronomy University of St Andrews North Haugh St Andrews KY16 9SS UK;
Computational Methods Group (CCS-2) Los Alamos National Laboratory P.O. Box 1663 Los Alamos NM 87545 USA;
gravitational waves - nuclear reactions; nucleosynthesis; abundances - stars: neutron;
机译:在两个中子恒星的合并之后,富含镧系元素的千克诺瓦的出现
机译:黑洞 - 中子星兼并的千龙瓦省排放。 I.查看角度依赖性电影
机译:Chandra X射线对中子星合并GW170817的观测:基洛诺瓦残留物的热X射线发射?
机译:GRB 060614中的R-Process Macronova / kilonova:中子星黑洞二进制文件合并的证据
机译:紧凑的物体自旋对寻找来自双星中子星和中子星-黑洞合并的引力波的影响。
机译:双中子星合并祖先产生的特殊低发光度短伽马射线爆发
机译:两颗中子星合并后出现富含镧系元素的新星