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Titlebook: Extreme Particle Acceleration in Microquasar Jets and Pulsar Wind Nebulae with the MAGIC Telescopes; Alba Fernández Barral Book 2018 Sprin

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發(fā)表于 2025-3-21 19:39:40 | 只看該作者 |倒序瀏覽 |閱讀模式
書目名稱Extreme Particle Acceleration in Microquasar Jets and Pulsar Wind Nebulae with the MAGIC Telescopes
編輯Alba Fernández Barral
視頻videohttp://file.papertrans.cn/321/320040/320040.mp4
概述Nominated as an outstanding PhD thesis by the Universitat Autònoma de Barcelona, Bellatara, Spain.Presents an extensive overview of various gamma-ray detection techniques, focusing on imaging atmosphe
叢書名稱Springer Theses
圖書封面Titlebook: Extreme Particle Acceleration in Microquasar Jets and Pulsar Wind Nebulae with the MAGIC Telescopes;  Alba Fernández Barral Book 2018 Sprin
描述.This exhaustive work sheds new light on unsolved questions in gamma-ray astrophysics. It presents not only a complete introduction to the non-thermal Universe, but also a description of the Imaging Atmospheric Cherenkov technique and the MAGIC telescopes. The Fermi-LAT satellite and the HAWC Observatory are also described, as results from both are included. The physics section of the book is divided into microquasars and pulsar wind nebulae (PWNe), and includes extended overviews of both. .In turn, the book discusses constraints on particle acceleration and gamma-ray production in microquasar jets, based on the analyses of MAGIC data on Cygnus X-1, Cygnus X-3 and V404 Cygni. Moreover, it presents the discovery of high-energy gamma-ray emissions from Cygnus X-1, using Fermi-LAT data. The book includes the first joint work between MAGIC, Fermi-LAT and HAWC, and discusses the hypothetical PWN nature of the targets in depth. It reports on a PWN population study that discusses, forthe first time, the importance of the surrounding medium for gamma-ray production, and in closing presents technical work on the first Large-Size-Telescope (LST; CTA Collaboration), along with a complete desc
出版日期Book 2018
關(guān)鍵詞Gamma Rays; Gamma-ray Astronomy; Pulsar Wind Nebulae; Microquasars and Binary Systems; Gamma-ray Detecti
版次1
doihttps://doi.org/10.1007/978-3-319-97538-2
isbn_softcover978-3-030-07371-8
isbn_ebook978-3-319-97538-2Series ISSN 2190-5053 Series E-ISSN 2190-5061
issn_series 2190-5053
copyrightSpringer Nature Switzerland AG 2018
The information of publication is updating

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沙發(fā)
發(fā)表于 2025-3-21 22:53:41 | 只看該作者
Microquasars, Binary Systems with?Powerful Jetsth 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 responsible of joining the dust and gas of the environment to give rise to the celestial objects.
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發(fā)表于 2025-3-22 00:55:44 | 只看該作者
2190-5053 orthe first time, the importance of the surrounding medium for gamma-ray production, and in closing presents technical work on the first Large-Size-Telescope (LST; CTA Collaboration), along with a complete desc978-3-030-07371-8978-3-319-97538-2Series ISSN 2190-5053 Series E-ISSN 2190-5061
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發(fā)表于 2025-3-22 08:07:58 | 只看該作者
Extreme Particle Acceleration in Microquasar Jets and Pulsar Wind Nebulae with the MAGIC Telescopes
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發(fā)表于 2025-3-22 17:02:54 | 只看該作者
Hajnalka Vaagen,Stein W. Wallaceth 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 responsible of joining the dust and gas of the environment to give rise to the celestial objects.
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發(fā)表于 2025-3-22 22:52:05 | 只看該作者
https://doi.org/10.1007/978-3-642-32030-9The 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.
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發(fā)表于 2025-3-23 04:59:01 | 只看該作者
https://doi.org/10.1007/978-3-322-82455-4Cygnus?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.
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發(fā)表于 2025-3-23 06:08:48 | 只看該作者
Cosmic Rays and Gamma-Ray AstrophysicsThe 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.
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