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Titlebook: Very-high-energy Gamma-ray Observations of Pulsar Wind Nebulae and Cataclysmic Variable Stars with M; Rubén López Coto Book 2017 Springer

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發(fā)表于 2025-3-21 16:09:26 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書目名稱Very-high-energy Gamma-ray Observations of Pulsar Wind Nebulae and Cataclysmic Variable Stars with M
編輯Rubén López Coto
視頻videohttp://file.papertrans.cn/983/982617/982617.mp4
概述Nominated as an outstanding PhD thesis by the Universitat Autònoma de Barcelona, Spain.Presents a state-of-the-art overview of the imaging atmospheric Cherenkov technique and the MAGIC telescopes.Offe
叢書名稱Springer Theses
圖書封面Titlebook: Very-high-energy Gamma-ray Observations of Pulsar Wind Nebulae and Cataclysmic Variable Stars with M;  Rubén López Coto Book 2017 Springer
描述This thesis is a comprehensive work that addresses many of the open questions currently being discusssed in the very-high-energy (VHE) gamma-ray community. It presents a detailed description of the MAGIC telescope together with a glimpse of the future Cherenkov Telescope Array (CTA). One section is devoted to the design, development and characterization of trigger systems for current and future imaging atmospheric Cherenkov telescopes. The book also features a state-of-the-art description of pulsar wind nebula (PWN) systems, the study of the multi-TeV spectrum of the Crab nebula, as well as the discovery of VHE gamma rays at the multiwavelength PWN 3C 58, which were sought at these wavelengths for more than twenty years. It also includes the contextualization of this discovery amongst the current population of VHE gamma-ray PWNe. Cataclysmic variable stars represent a new source of gamma ray energies, and are also addressed here. In closing, the thesis reports on the systematic search for VHE gamma-ray emissions of AE Aquarii in a multiwavelength context and the search for VHE gamma-ray variability of novae during outbursts at different wavelengths..?.
出版日期Book 2017
關(guān)鍵詞Gamma Ray observation; Pulsar Wind Nebulae; Cataclysmic Variable Stars; Imaging Atmospheric Cherenkov T
版次1
doihttps://doi.org/10.1007/978-3-319-44751-3
isbn_softcover978-3-319-83128-2
isbn_ebook978-3-319-44751-3Series ISSN 2190-5053 Series E-ISSN 2190-5061
issn_series 2190-5053
copyrightSpringer International Publishing AG, part of Springer Nature 2017
The information of publication is updating

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Very-high-energy Gamma-ray Observations of Pulsar Wind Nebulae and Cataclysmic Variable Stars with M978-3-319-44751-3Series ISSN 2190-5053 Series E-ISSN 2190-5061
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Summary and Concluding RemarksIn this chapter I give a summary of all the results found on this thesis and also give future prospects for the observation of the phenomena studied on this thesis.
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Short Introduction to Cosmic Ray and ,-Ray Astronomysources producing them. I also give an introduction to gamma-ray astronomy, the detection techniques and the mechanisms producing gamma rays. I finally describe all the sources known to date where gamma rays are produced.
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