Revealing the Most Energetic Light from Pulsars and Their Nebulae / Springer Theses (PDF)
(Sprache: Englisch)
>100 GeV, emissions from millisecond pulsars using the Large Area Telescope on board the Fermi satellite, as well as a study on the promising Pulsar Wind Nebula candidate PSR J0631.
The observation of VHE gamma rays is essential to studying the...
The observation of VHE gamma rays is essential to studying the...
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>100 GeV, emissions from millisecond pulsars using the Large Area Telescope on board the Fermi satellite, as well as a study on the promising Pulsar Wind Nebula candidate PSR J0631.
The observation of VHE gamma rays is essential to studying the non-thermal sources of radiation 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.
Bibliographische Angaben
- Autor: David Carreto Fidalgo
- 2019, 1st ed. 2019, 208 Seiten, Englisch
- Verlag: Springer-Verlag GmbH
- ISBN-10: 3030241947
- ISBN-13: 9783030241940
- Erscheinungsdatum: 17.07.2019
Abhängig von Bildschirmgröße und eingestellter Schriftgröße kann die Seitenzahl auf Ihrem Lesegerät variieren.
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- Größe: 9.21 MB
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Englisch
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