| 书目名称 | Very-high-energy Gamma-ray Observations of Pulsar Wind Nebulae and Cataclysmic Variable Stars with M | | 编辑 | Rubén López Coto | | 视频video | | | 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 | | 丛书名称 | Springer Theses | | 图书封面 |  | | 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 | | 关键词 | Gamma Ray observation; Pulsar Wind Nebulae; Cataclysmic Variable Stars; Imaging Atmospheric Cherenkov T | | 版次 | 1 | | doi | https://doi.org/10.1007/978-3-319-44751-3 | | isbn_softcover | 978-3-319-83128-2 | | isbn_ebook | 978-3-319-44751-3Series ISSN 2190-5053 Series E-ISSN 2190-5061 | | issn_series | 2190-5053 | | copyright | Springer International Publishing AG, part of Springer Nature 2017 |
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发表于 2025-3-21 16:09:26
