Английская Википедия:High-energy astronomy

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Версия от 09:53, 21 марта 2024; EducationBot (обсуждение | вклад) (Новая страница: «{{Английская Википедия/Панель перехода}} '''High-energy astronomy''' is the study of astronomical objects that release electromagnetic radiation of highly energetic wavelengths. It includes X-ray astronomy, gamma-ray astronomy, extreme UV astronomy, neutrino astronomy, and studies of cosmic rays. The physical study of these phenomena is referr...»)
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High-energy astronomy is the study of astronomical objects that release electromagnetic radiation of highly energetic wavelengths. It includes X-ray astronomy, gamma-ray astronomy, extreme UV astronomy, neutrino astronomy, and studies of cosmic rays. The physical study of these phenomena is referred to as high-energy astrophysics.[1]

Astronomical objects commonly studied in this field may include black holes, neutron stars, active galactic nuclei, supernovae, kilonovae, supernova remnants, and gamma-ray bursts.

Missions

Some space and ground-based telescopes that have studied high energy astronomy include the following:[2] Шаблон:Div col

References

Шаблон:Reflist

External links

Шаблон:Astronomy navbox

Шаблон:Astronomy-stub

Партнерские ресурсы
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  1. ↑ Шаблон:Cite web
  2. ↑ Шаблон:Cite web
Источник — http://wikihandbk.com/ruwiki/index.php?title=Английская_Википедия:High-energy_astronomy&oldid=15237758