Titlebook: Revealing the Most Energetic Light from Pulsars and Their Nebulae; David Carreto Fidalgo Book 2019 Springer Nature Switzerland AG 2019 Cra

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Book 2019iation in our Universe. Rotating neutron stars, also known as pulsars, are an extreme source class known to emit VHE gamma rays. However, to date only two pulsars have been detected with emissions above 100 GeV, and our understanding of their emission mechanism is still lacking. .

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David Carreto Fidalgon unterscheiden.. Dabei hat sich die auf . (1986) und (1989) zurückgehende Free-Cash-flow-Theorie als dominierender Erklärungsansatz für Going Private-Transaktionen am US-amerikanischen Kapitalmarkt herausgebildet.. Ihr zufolge sind Going Private-Unternehmen vor allem durch hohe freie Cash-flows gek

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Cherenkov Telescopes and MAGICThe first source of very-high-energy (.) gamma rays, the Crab nebula, was firmly detected by the Whipple collaboration in the 1980s [.]. Their pioneering instrument and analysis method became the basic concept in the field of Imaging Atmospheric Cherenkov Telescopes (.s) and paved the way for todays third generation telescopes.

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Search for the Next Very-High-Energy PulsarWhile over 200 pulsars are known to emit gamma rays in the MeV to GeV regime, only two pulsars have been detected at Very High Energy (., . GeV) so far: the Crab pulsar in the Northern Hemisphere and the Vela pulsar in the Southern Hemisphere.

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