Polarization in the inner region of pulsar wind nebulae

Astronomy and Astrophysics

Volumn 443, Issue 2, 2005, Pages 519-524

  Bucciantini, N ^a   Del Zanna, L ^b   Amato, E ^c   Volpi, D ^b  

^a UNIVERSITY OF CALIFORNIA   (United States)

^b UNIVERSITY OF FLORENCE   (Italy)

^c INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

Author keywords

ISM: supernova remnants; Magnetohydrodynamics (MHD); Polarization; Radiation mechanisms: non thermal; Relativity; Stars: pulsars: general

Indexed keywords

COMPUTER SIMULATION; LIGHT POLARIZATION; POLARIZATION; SYNCHROTRON RADIATION; VELOCITY MEASUREMENT;

ISM: SUPERNOVA REMNANTS; PULSAR WIND NEBULAE (PWNE); RADIATION MECHANISMS: NON-THERMAL; STARS: PULSARS: GENERAL;

ASTRONOMY;

EID: 27844554354     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20053667     Document Type: Article

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