Neutrino transport in strongly magnetized proto-neutron stars and the origin of pulsar kicks: The effect of asymmetric magnetic field topology

Astrophysical Journal

Volumn 505, Issue 2 PART I, 1998, Pages 844-853

  Lai, Dong ^a   Qian, Yong Zhong ^b  

^a Department of Population Medicine and Diagnostic Sciences   (United States)

^b CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

Author keywords

Dense matter; Magnetic fields; Pulsars: General; Radiative transfer stars: Neutron; Supernovae: General

Indexed keywords

EID: 26144480921     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/306203     Document Type: Article

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