Theory of high-energy emission from the pulsar/be star system PSR 1259-63. I. radiation mechanisms and interaction geometry

Astrophysical Journal

Volumn 477, Issue 1 PART I, 1997, Pages 439-464

  Tavani, Marco ^a   Arons, Jonathan ^b,c  

^a Och Spine at New York Presbyterian Hospitals   (United States)

^b UNIVERSITY OF CALIFORNIA   (United States)

^c LAWRENCE LIVERMORE NATIONAL LABORATORY   (United States)

Author keywords

Binaries: Close; Pulsars: Individual (psr b1259 63); Radiation mechanisms: Nonthermal; Shock waves; Stars: Emission line, be x rays: Stars

Indexed keywords

EID: 21744438004     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/303676     Document Type: Article

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