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mission for X-ray astronomy, taking its place in the fleet of "Great Observatories." Chandra Spacecraft Components; Who we are. NASA's Chandra X-ray Observatory is a telescope specially designed to detect X-ray emission from very hot regions of the Universe such as exploded stars, clusters of galaxies, and matter around black holes.
An ultraluminous X-ray source ( ULX) is an astronomical source of X-rays that is less luminous than an active galactic nucleus but is more consistently luminous than any known stellar process (over 10 39 erg /s, or 10 32 watts ), assuming that it radiates isotropically (the same in all directions). Typically there is about one ULX per galaxy in ...
14 de ago. de 2015 · PRAXyS Science. PRAXyS, the Polarimeter for Relativistic Astrophysical X-ray Sources, will use X-ray telescopes to explore the shape of space that has been distorted by a spinning black hole's gravity, and probe the structure and effects of the magnetic field around neutron stars. Current missions cannot do this because the required angular ...
This is an audio version of the Wikipedia Article:https://en.wikipedia.org/wiki/Astrophysical_X-ray_source00:01:37 1 Galaxy clusters00:02:54 2 Quasars00:04:4...
Astronomical X-ray sources: X-ray astronomy, Celestial X-ray source, X-1 X-ray source, Astrophysical X-ray source : Source: Wikipedia: Amazon.es: Libros Saltar al contenido principal .es
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Cygnus X-1 (abbreviated Cyg X-1) is a galactic X-ray source in the constellation Cygnus and was the first such source widely accepted to be a black hole. It was discovered in 1965 during a rocket flight and is one of the strongest X-ray sources detectable from Earth, producing a peak X-ray flux density of 2.3 × 10 −23 W/(m 2 ⋅Hz) (2.3 × 10 3 jansky).
27 de may. de 2022 · Abstract. Grazing-incidence X-ray optics have revolutionized X-ray astrophysics. The ability to concentrate flux to a tiny detection region provides a dramatic reduction in background and a consequent very large improvement in sensitivity. The X-ray optics also permit use of small-format, high-performance focal-plane detectors and, of course ...
