Discovery of small scale filaments in SN 1006 - New approach for understanding cosmic ray acceleration

Details Discovery of small scale filaments in SN 1006 - New approach for understanding cosmic ray acceleration Discovery of small scale filaments in SN 1006 - New approach for understanding cosmic ray acceleration

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004asthe..97..679b&link_type=abstract

The Astronomical Herald (ISSN 0374-2466), Vol. 97, No. 12, p. 679 - 686 (2004)

Astronomy and Astrophysics

Astronomy

1

Supernova Remnants, Filaments, Cosmic Rays, Acceleration

Scientific paper

With excellent spatial resolution of the X-ray satellite Chandra, we discovered synchrotron X-rays in the supernova remnant SN 1006, which concentrate on very thin filamental structure. In order to illustrate the thin filaments with diffusive shock acceleration mechanism (DSA), we need (I) perpendicular magnetic field to the shock normal with the strength of interstellar magnetic field or (II) very compressed parallel one. This method is a new approach to understanding the DSA.

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