Relativistic jets: an overview of recent progress
Despite their different nature and physics, blazars and γ ray bursts have in common very powerful relativistic jets, which make them the most luminous sources in the Universe. The energy extraction from the central compact object, the jet collimation, the role and geometry of the magnetic fields, th...
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I19-R120-10915-1678332024-07-05T20:02:27Z http://sedici.unlp.edu.ar/handle/10915/167833 Relativistic jets: an overview of recent progress Pian, Elena 2015-10 2016 2024-07-05T18:10:38Z en Ciencias Astronómicas blazars gammaray burst jets relativistic jets: Despite their different nature and physics, blazars and γ ray bursts have in common very powerful relativistic jets, which make them the most luminous sources in the Universe. The energy extraction from the central compact object, the jet collimation, the role and geometry of the magnetic fields, the structure of the jet itself represent still big enough questions that a complete paradigm cannot yet be drawn. This article is concerned with the main observational facts about blazars and gammaray burst jets, based on multi-wavelength campaigns, and on the clues one can glean from these on jet formation, behavior and powering. The future generation of telescopes and instruments and the contributions from multi-messenger investigation (astroparticle diagnostics and gravitational waves) will warrant further significant progress. Facultad de Ciencias Astronómicas y Geofísicas Objeto de conferencia Objeto de conferencia http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) application/pdf 3-12 |
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Universidad Nacional de La Plata |
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R-120 |
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SEDICI (UNLP) |
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Inglés |
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Ciencias Astronómicas blazars gammaray burst jets relativistic jets: |
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Ciencias Astronómicas blazars gammaray burst jets relativistic jets: Pian, Elena Relativistic jets: an overview of recent progress |
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Ciencias Astronómicas blazars gammaray burst jets relativistic jets: |
description |
Despite their different nature and physics, blazars and γ ray bursts have in common very powerful relativistic jets, which make them the most luminous sources in the Universe. The energy extraction from the central compact object, the jet collimation, the role and geometry of the magnetic fields, the structure of the jet itself represent still big enough questions that a complete paradigm cannot yet be drawn. This article is concerned with the main observational facts about blazars and gammaray burst jets, based on multi-wavelength campaigns, and on the clues one can glean from these on jet formation, behavior and powering. The future generation of telescopes and instruments and the contributions from multi-messenger investigation (astroparticle diagnostics and gravitational waves) will warrant further significant progress. |
format |
Objeto de conferencia Objeto de conferencia |
author |
Pian, Elena |
author_facet |
Pian, Elena |
author_sort |
Pian, Elena |
title |
Relativistic jets: an overview of recent progress |
title_short |
Relativistic jets: an overview of recent progress |
title_full |
Relativistic jets: an overview of recent progress |
title_fullStr |
Relativistic jets: an overview of recent progress |
title_full_unstemmed |
Relativistic jets: an overview of recent progress |
title_sort |
relativistic jets: an overview of recent progress |
publishDate |
2015 |
url |
http://sedici.unlp.edu.ar/handle/10915/167833 |
work_keys_str_mv |
AT pianelena relativisticjetsanoverviewofrecentprogress |
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1807223572832190464 |