A model of polarized X-ray emission from twinkling synchrotron supernova shells

Monthly Notices of the Royal Astronomical Society

Volumn 399, Issue 3, 2009, Pages 1119-1125

  Bykov, A M ^a   Uvarov, Yu A ^a   Bloemen, J B G M ^b   Den Herder, J W ^b   Kaastra, J S ^b  

^a IOFFE INSTITUTE   (Russian Federation)

^b SRON NETHERLANDS INSTITUTE FOR SPACE RESEARCH   (Netherlands)

Author keywords

Polarization; Radiation mechanisms: non thermal; Shock waves; Supernova remnants; X rays: ISM

Indexed keywords

ELECTROMAGNETIC WAVE EMISSION; MAGNETIC FIELDS; SHOCK WAVES; TELLURIUM COMPOUNDS; X RAY SCATTERING;

DIFFUSIVE SHOCK ACCELERATIONS; ENERGY; FLUCTUATING FIELDS; NONTHERMAL EMISSION; RADIATION MECHANISMS: NONTHERMAL; SHOCK-WAVES; SUPERNOVA REMNANTS; SUPERNOVA SHELLS; X RAYS: ISM; X-RAY EMISSION;

POLARIZATION;

EID: 70350064103     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2009.15348.x     Document Type: Article

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