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dc.date.accessioned 2024-07-05T18:10:38Z
dc.date.available 2024-07-05T18:10:38Z
dc.date.issued 2016
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/167833
dc.description.abstract 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. en
dc.format.extent 3-12 es
dc.language en es
dc.subject blazars es
dc.subject gammaray burst jets es
dc.subject relativistic jets: es
dc.title Relativistic jets: an overview of recent progress en
dc.type Objeto de conferencia es
sedici.identifier.isbn 978-987-24948-3-4 es
sedici.creator.person Pian, Elena es
sedici.subject.materias Ciencias Astronómicas es
sedici.description.fulltext true es
mods.originInfo.place Facultad de Ciencias Astronómicas y Geofísicas es
sedici.subtype Objeto de conferencia es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.date.exposure 2015-10
sedici.relation.event High-Energy Phenomena tn Relativistic Outflows V (La Plata, 5 al 8 de octubre de 2015) es
sedici.description.peerReview peer-review es
sedici.relation.isRelatedWith https://sedici.unlp.edu.ar/handle/10915/167830 es
sedici.relation.bookTitle Proceedings of the High-Energy Phenomena in Relativistic Outflows V meeting es


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