A model for non high energy Gamma Ray Bursts and sources of ultra high energy cosmic rays: Super strongly magnetized milli-second pulsar formed from a (C+O) star and a neutron star (black hole) close binary system

Progress of Theoretical Physics

Volumn 100, Issue 5, 1998, Pages 921-929

  Nakamura, Takashi ^a  

^a KYOTO UNIVERSITY   (Japan)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0040843495     PISSN: 0033068X     EISSN: None     Source Type: Journal    
DOI: 10.1143/PTP.100.921     Document Type: Article

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