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The supernova remnant SN 1006 as a Galactic particle accelerator
Published 2022-08-01“…Here, the authors show that SN 1006 remnant is an efficient source of cosmic rays, providing observational support for the quasi-parallel acceleration mechanism.…”
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Magnetic Structures and Turbulence in SN 1006 Revealed with Imaging X-Ray Polarimetry
Published 2023-01-01“…We report the X-ray polarization distribution in the northeastern shell of SN 1006 from a 1 Ms observation with the Imaging X-ray Polarimetry Explorer. …”
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Hunting for the progenitor of SN 1006: High resolution spectroscopic search with the FLAMES instrument
Published 2012“…We find no star consistent with the traditional accretion scenario in SN1006.…”
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ENVIRONMENTAL LIMITS ON THE NONRESONANT COSMIC-RAY CURRENT-DRIVEN INSTABILITY
Published 2008“…Limits on the growth of the nonresonant mode in SN1006 and RX J1713.7-3946 are presented. © 2008 World Scientific Publishing Company.…”
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Cosmic ray acceleration in young supernova remnants
Published 2013“…We also find that for a typical background magnetic field strength of 5 μG the instability is quenched in about 1000 years, making SN1006 just at the border of candidates for cosmic ray acceleration to high energies. © 2013 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society.…”
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