Magnetic Rayleigh-Taylor instability for Pulsar Wind Nebulae in expanding Supernova Remnants

Astronomy and Astrophysics

Volumn 423, Issue 1, 2004, Pages 253-265

  Bucciantini, N ^a,b   Amato, E ^c   Bandiera, R ^c   Blondin, J M ^b   Del Zanna, L ^a  

^a UNIVERSITY OF FLORENCE   (Italy)

^b NORTH CAROLINA STATE UNIVERSITY   (United States)

^c INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

Author keywords

Instabilities; ISM: supernova remnants; Magnetohydrodynamics (MHD); Stars: pulsars: general; Stars: winds, outflows

Indexed keywords

COOLING; ELECTROMAGNETISM; MAGNETIC FIELDS; MAGNETOHYDRODYNAMICS; PARAMETER ESTIMATION; TORQUE; ULTRAVIOLET RADIATION; WIND;

ISM:SUPERNOVA REMNANTS; NEBULA EVOLUTION; PULSAR WIND NEBULA (PWN); STARS:PULSARS:GENERAL;

ASTROPHYSICS;

EID: 4043094956     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20040360     Document Type: Article

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