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Extreme Particle Acceleration in Microquasar Jets and Pulsar Wind Nebulae with the MAGIC Telescopes

Part of the Springer Theses Book Series

DOI: 10.1007/978-3-319-97538-2

ISBN: 978-3-319-97537-5

Publisher: Springer International Publishing - Springer Journals

Oct 13, 2018

1 - 10 of 11 Chapters

LitStream

Cosmic Rays and Gamma-Ray Astrophysics

Fernández Barral, Alba

Pages: 3 –16

[The history of gamma-ray astronomy, or the non-thermal astrophysics in general, is quite recent. It goes back only to the 20th century, when the physicist Victor Hess discovered what was thought to be a new kind of radiation that would forever change our conception of the Universe.]
LitStream

Gamma-Ray Telescopes

Fernández Barral, Alba

Pages: 17 –79

[In this chapter, I will describe in detail both hardware of the Major Atmospheric Gamma-ray Imaging Cherenkov (MAGIC) telescopes and the software used in the analysis of the data. Moreover, I will give an overview of the planned CTA, future generation of Cherenkov telescopes. Although this...
LitStream

Microquasars, Binary Systems with Powerful Jets

Fernández Barral, Alba

Pages: 83 –103

[Our Galaxy contains hundred billions of stars with very different features, masses, size and ages. The understanding of their birth, evolution and death was, and still remains to be, a goal to achieve for the astronomers. The life of the stars begins within molecular clouds, where gravity is...
LitStream

Cygnus X-1

Fernández Barral, Alba

Pages: 105 –131

[Cygnus X-1 is one of the brightest and most studied X-ray sources in our Galaxy and a firmly established stellar-mass BH X-ray binary system.]
LitStream

Cygnus X-3

Fernández Barral, Alba

Pages: 133 –150

[Cygnus X-3, discovered 50 years ago (Giacconi et al. 1967), is one of the brightest X-ray sources in our Galaxy and the strongest radio source among the X-ray binaries, displaying two-sided transient powerful relativistic radio jets (Martí et al. 2001; Miller-Jones et al. 2004).]
LitStream

V404 Cygni

Fernández Barral, Alba

Pages: 151 –159

[V404 Cygni is a low-mass microquasar composed of a 8–15 M\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek}...
LitStream

Introduction to Pulsar Wind Nebulae

Fernández Barral, Alba

Pages: 163 –172

[The ejected material by a SN explosion interacts with the surrounding environment, giving rise to a new astrophysical object known as SNR (for a review of this matter, I refer the reader to (Reynolds 2008) and to Appendix A for more information on the first evolutionary phase).]
LitStream

Follow-Up Studies of HAWC Sources

Fernández Barral, Alba

Pages: 173 –188

[On the 15th of April 2016, the HAWC Collaboration released a preliminary second catalog (2HWC) with 39 TeV sources, from which 19 have no association with any known HE or VHE source (within an angular distance of 0.5\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym}...
LitStream

PWN Studies Around High Spin-Down Power Fermi-LAT Pulsars

Fernández Barral, Alba

Pages: 189 –201

[As shown in Chap. 7, pulsars are highly magnetized rotating neutron stars born in SN explosions which are constantly releasing their rotational energy in the form of relativistic Poynting and particle flux, the so-called pulsar wind. This wind interacts with the ISM, giving rise to a termination...
LitStream

Quality Control of LST Camera Subsystems

Fernández Barral, Alba

Pages: 205 –222

[CTA intends to reach up to 10 times better sensitivity (around 1 TeV) than the current IACTs and extend the energy range. The LST are the responsible for the sensitivity below \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts}...

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