Origin of the heavy elements in binary neutron-star mergers from a gravitational-wave event

被引：0
|
作者：
Daniel Kasen
Brian Metzger
Jennifer Barnes
Eliot Quataert
Enrico Ramirez-Ruiz
机构：
[1] and Theoretical Astrophysics Center,Departments of Physics and Astronomy
[2] University of California,Nuclear Science Division
[3] Berkeley,Department of Physics and Columbia Astrophysics Laboratory
[4] Lawrence Berkeley National Laboratory,Department of Astronomy
[5] Columbia University,undefined
[6] University of Santa Cruz,undefined
[7] DARK,undefined
[8] Niels Bohr Institute,undefined
[9] University of Copenhagen,undefined
来源：
Nature | 2017年 / 551卷
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摘要：
Modelling the electromagnetic emission of kilonovae enables the mass, velocity and composition (with some heavy elements) of the ejecta from a neutron-star merger to be derived from the observations.
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页码：80 / 84
页数：4
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