Observational constraints on the modelling of SN 1006
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/413/3/1643/2868294/mnras0413-1643.pdf
Reference33 articles.
1. First detection of VHEγ-rays from SN 1006 by HESS
2. A detailed spectral and morphological study of the gamma-ray supernova remnant RX J1713.7–3946 with HESS
3. Evidence of a Curved Synchrotron Spectrum in the Supernova Remnant SN 1006
4. X-ray synchrotron emission from supernova remnants
5. Suzaku Wide-Band Observations of SN 1006
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1. Evolution and observational signatures of the cosmic ray electron spectrum in SN 1006;Monthly Notices of the Royal Astronomical Society;2020-10-02
2. Constraining the coherence scale of the interstellar magnetic field using TeV gamma-ray observations of supernova remnants;Monthly Notices of the Royal Astronomical Society;2020-06-12
3. Radio polarization maps of shell-type SNRs – II. Sedov models with evolution of turbulent magnetic field;Monthly Notices of the Royal Astronomical Society;2017-05-18
4. Supernova of 1006 (G327.6+14.6);Handbook of Supernovae;2017
5. Supernova of 1006 (G327.6+14.6);Handbook of Supernovae;2017
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