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3D MHD simulation of polarized emission in SN 1006
(Oxford University Press, 2015-02)
We use three-dimensional magnetohydrodynamic simulations to model the supernova remnant SN 1006. From our numerical results, we have carried out a polarization study, obtaining synthetic maps of the polarized intensity, ...
On the Radio Polarization Signature of Efficient and Inefficient Particle Acceleration in Supernova Remnant SN 1006
(Iop Publishing, 2013-04)
Radio polarization observations provide essential information on the degree of order and orientation of magnetic fields, which themselves play a key role in the particle acceleration processes that take place in supernova ...
Mass loss from the progenitor of SN 1006?
(Universidad Nacional Autónoma de México. Instituto de Astronomía, 2008)
Shock-Cloud Interaction and Particle Acceleration in the Southwestern Limb of SN 1006
(Iop Publishing, 2014-02)
The supernova remnant SN 1006 is a powerful source of high-energy particles and evolves in a relatively tenuous and uniform environment despite interacting with an atomic cloud in its northwestern limb. The X-ray image of ...
Predicted gamma-ray image of SN 1006 due to inverse Compton emission
(Oxford University Press, 2009-12)
We propose a method to synthesize the inverse Compton (IC) γ-ray image of a supernova remnant starting from the radio (or hard X-ray) map and using results of the spatially resolved X-ray spectral analysis. The method ...
The neutral gas environment of the young supernova remnant SN 1006 (G327.6+14.6)
(EDP Sciences, 2002-06)
Using the Australia Telescope Compact Array, we have carried out a survey of the H i emission in the direction of the bilateral supernova remnant (SNR) SN 1006 (G327.6+14.6). The angular resolution of the data is 4.07×3.00, ...
Morphological evidence for azimuthal variations of the cosmic ray ion acceleration at the blast wave of SN 1006
(IOP Publishing, 2008-12)
Using radio, X-ray and optical observations, we present evidence for morphological changes due to efficient cosmic ray ion acceleration in the structure of the southeastern region of the supernova remnant SN 1006. SN 1006 ...
Thermal emission, shock modification, and X-ray emitting ejecta in SN 1006
(EDP Sciences, 2009-12)
Context: Efficient particle acceleration can modify the structure of supernova remnants. We present the results of a combined analysis of the XMM-Newton EPIC archive observations of SN 1006. Aims: We attempt to describe ...
Aspect angle for interstellar magnetic field in SN 1006
(Oxford University Press, 2009-12)
A number of important processes taking place around strong shocks in supernova remnants (SNRs) depend on the shock obliquity. The measured synchrotron flux is a function of the aspect angle between interstellar magnetic ...