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  1. OA@INAF
  2. PRODOTTI RICERCA INAF
  3. 1 CONTRIBUTI IN RIVISTE (Journal articles)
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Please use this identifier to cite or link to this item: http://hdl.handle.net/20.500.12386/29482
Title: The Crab nebula in the light of three-dimensional relativistic MHD simulations
Authors: Del Zanna, L.
Olmi, Barbara 
AMATO, Elena 
BUCCIANTINI, NICCOLO' 
Mignone, A.
Issue Date: 2019
Journal: RENDICONTI LINCEI. SCIENZE FISICHE E NATURALI 
Number: 30
Issue: S1
First Page: 93
Abstract: Pulsar wind nebulae inside young supernova remnants, and in particular the Crab nebula, are probably the best laboratories for high-energy astrophysics and relativistic plasma physics. They have been modeled numerically for more than a decade through multi-dimensional relativistic MHD simulations, relying on axial symmetry until a few years ago while currently using full three-dimensional simulations employing adaptive meshes. Here, we discuss the most recent findings, especially those obtained by our Arcetri group, focusing on the problem of magnetic field dissipation inside the nebula.
URI: http://hdl.handle.net/20.500.12386/29482
URL: https://link.springer.com/article/10.1007/s12210-019-00759-y
ISSN: 2037-4631
DOI: 10.1007/s12210-019-00759-y
Bibcode ADS: https://ui.adsabs.harvard.edu/abs/2019RLSFN.tmp....1D/abstract
Fulltext: open
Appears in Collections:1.01 Articoli in rivista

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DelZanna2019_Article_TheCrabNebulaInTheLightOfThree.pdf[Administrators only]881.58 kBAdobe PDF
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