The role of superluminal electromagnetic waves in pulsar wind termination shocks

Astrophysical Journal

Volumn 770, Issue 1, 2013, Pages

  Amano, Takanobu ^a   Kirk, John G ^b  

^a UNIVERSITY OF TOKYO   (Japan)

^b MAX PLANCK INSTITUT FÜR KERNPHYSIK   (Germany)

Author keywords

plasmas; pulsars: general; stars: winds, outflows; waves

Indexed keywords

EID: 84878319193     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/770/1/18     Document Type: Article

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