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  2. Astrophysical X-ray source - Wikipedia

    en.wikipedia.org/wiki/Astrophysical_X-ray_source

    The Chandra X-ray image is of the quasar PKS 1127-145, a highly luminous source of X-rays and visible light about 10 billion light years from Earth. An enormous X-ray jet extends at least a million light years from the quasar. Image is 60 arcsec on a side. RA 11h 30 m 7.10s Dec −14° 49' 27" in Crater. Observation date: 28 May 2000.

  3. X-ray astronomy - Wikipedia

    en.wikipedia.org/wiki/X-ray_astronomy

    Within the constellations Orion and Eridanus and stretching across them is a soft X-ray "hot spot" known as the Orion-Eridanus Superbubble, the Eridanus Soft X-ray Enhancement, or simply the Eridanus Bubble, a 25° area of interlocking arcs of Hα emitting filaments. Soft X-rays are emitted by hot gas (T ~ 2–3 MK) in the interior of the ...

  4. History of X-ray astronomy - Wikipedia

    en.wikipedia.org/wiki/History_of_X-ray_astronomy

    Some 2 dozen known X-ray sources were monitored—some for more than 100 days—and a number of new X-ray transients were discovered. The Diffuse X-ray Spectrometer (DXS) STS-54 package was flown as an attached payload in January, 1993 to obtain spectra of the diffuse soft X-ray background. DXS obtained the first-ever high resolution spectra of ...

  5. X-ray - Wikipedia

    en.wikipedia.org/wiki/X-ray

    Natural color X-ray photogram of a wine scene. Note the edges of hollow cylinders as compared to the solid candle. William Coolidge explains medical imaging and X-rays.. An X-ray (also known in many languages as Röntgen radiation) is a form of high-energy electromagnetic radiation with a wavelength shorter than those of ultraviolet rays and longer than those of gamma rays.

  6. Astronomy - Wikipedia

    en.wikipedia.org/wiki/Astronomy

    X-ray jet made from a supermassive black hole found by NASA's Chandra X-ray Observatory, made visible by light from the early Universe. X-ray astronomy uses X-ray wavelengths. Typically, X-ray radiation is produced by synchrotron emission (the result of electrons orbiting magnetic field lines), thermal emission from thin gases above 10 7 (10 ...

  7. X-ray binary - Wikipedia

    en.wikipedia.org/wiki/X-ray_binary

    X-ray binaries are a class of binary stars that are luminous in X-rays. The X-rays are produced by matter falling from one component, called the donor (usually a relatively common main sequence star ), to the other component, called the accretor , which is either a neutron star or black hole .

  8. Cosmic ray spallation - Wikipedia

    en.wikipedia.org/wiki/Cosmic_ray_spallation

    The x-process in cosmic rays is the primary means of nucleosynthesis for the five stable isotopes of lithium, beryllium, and boron. [2] As the proton–proton chain reaction cannot proceed beyond 4 He due to the unbound nature of 5 He and 5 Li, [ 3 ] and the triple-alpha process skips over all species between 4 He and 12 C, these elements are ...

  9. Category:History of X-rays - Wikipedia

    en.wikipedia.org/wiki/Category:History_of_X-rays

    Pages in category "History of X-rays" The following 2 pages are in this category, out of 2 total. This list may not reflect recent changes. H. History of X-ray ...