Intermediate-mass Elements in Young Supernova Remnants Reveal Neutron Star Kicks by Asymmetric Explosions

The birth properties of neutron stars (NSs) yield important information about the still-debated physical processes that trigger the explosion as well as on intrinsic neutron-star physics. These properties include the high space velocities of young neutron stars with average values of several 100 km...

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Veröffentlicht in:	The Astrophysical journal 2018-03, Vol.856 (1), p.18
Hauptverfasser:	Katsuda, Satoru, Morii, Mikio, Janka, Hans-Thomas, Wongwathanarat, Annop, Nakamura, Ko, Kotake, Kei, Mori, Koji, Müller, Ewald, Takiwaki, Tomoya, Tanaka, Masaomi, Tominaga, Nozomu, Tsunemi, Hiroshi
Format:	Artikel
Sprache:	eng
Schlagworte:	Acceleration Astrophysics Asymmetry Calcium Chemical elements Ejection Explosions ISM: supernova remnants Magnetic fields methods: data analysis Neutrinos Neutron stars Neutrons Nuclear physics Organic chemistry Physics Stars & galaxies stars: neutron Stellar evolution Stellar magnetic fields Supernova Supernova remnants techniques: imaging spectroscopy X-ray measurements X-rays: general
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