The keV-TeV connection in gamma-ray binaries

The keV-TeV connection in gamma-ray binaries

Gamma-ray binaries are systems that comprise a young, massive star and a compact object that can be either a young pulsar or a black hole. They emit radiation from radio up to tens of TeV and show flux variability along the whole electromagnetic spectrum. For three of the four detected gamma-ray bin...

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Bibliographic Details
Main Author: Zabalza de Torres, Victor
Other Authors: Paredes i Poy, Josep Maria
Format: Doctoral Thesis
Language:English
Published: Universitat de Barcelona 2011
Subjects:
Estels binaris
Double stars
Estrellas dobles
Estels binaris de raigs x
Binarias de rayos X
X-ray binaries
Astronomia de raigs gamma
Astronomía de rayos gamma
Gamma ray astronomy
Vent estel.lar
Viento estelar
Stellar wind
Mecanisme de radiació no tèrmica
Mecanismo de radiación no térmica
Non-thermal radiation mechanism
Ciències Experimentals i Matemàtiques
52
Online Access:http://hdl.handle.net/10803/33649

Internet

http://hdl.handle.net/10803/33649

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