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  2. Crab Nebula - Wikipedia

    en.wikipedia.org/wiki/Crab_Nebula

    The Crab Pulsar, a neutron star 28–30 kilometres (17–19 mi) across with a spin rate of 30.2 times per second, lies at the center of the Crab Nebula. The star emits pulses of radiation from gamma rays to radio waves .

  3. Crab Pulsar - Wikipedia

    en.wikipedia.org/wiki/Crab_Pulsar

    The Crab Pulsar (PSR B0531+21 or Baade's Star) is a relatively young neutron star.The star is the central star in the Crab Nebula, a remnant of the supernova SN 1054, which was widely observed on Earth in the year 1054.

  4. Crab (unit) - Wikipedia

    en.wikipedia.org/wiki/Crab_(unit)

    The Crab Nebula, and the Crab Pulsar within it, is an intense space X-ray source. It is used as a standard candle in the calibration procedure of X-ray instruments in space. However, because of the Crab Nebula's variable intensity at different X-ray energies, conversion of the Crab to another units depends on the X-ray energy range of interest.

  5. NASA's Hubble captures stunning photos of the Crab Nebula's ...

    www.aol.com/article/2016/07/07/nasas-hubble...

    It spins at a rate of 30 times per second, spewing energy beams and taking on a decidedly pulsating appearance. NASA's Hubble captures stunning photos of the Crab Nebula's 'beating heart' Skip to ...

  6. Near-Earth supernova - Wikipedia

    en.wikipedia.org/wiki/Near-Earth_supernova

    The Crab Nebula is a pulsar wind nebula associated with the 1054 supernova.It is located about 6,500 light-years from the Earth. [1]A near-Earth supernova is an explosion resulting from the death of a star that occurs close enough to the Earth (roughly less than 10 to 300 parsecs [30 to 1000 light-years] away [2]) to have noticeable effects on Earth's biosphere.

  7. Synchrotron radiation - Wikipedia

    en.wikipedia.org/wiki/Synchrotron_radiation

    Pulsed emission gamma-ray radiation from the Crab has recently been observed up to ≥25 GeV, [21] probably due to synchrotron emission by electrons trapped in the strong magnetic field around the pulsar. Polarization in the Crab nebula [22] at energies from 0.1 to 1.0 MeV, illustrates this typical property of synchrotron radiation.

  8. Cosmic dust - Wikipedia

    en.wikipedia.org/wiki/Cosmic_dust

    Supernova remnants, on the other hand, like the Crab Nebula, are characterized as nonthermal emission (synchrotron radiation). Some of the better known dusty regions in the Universe are the diffuse nebulae in the Messier catalog, for example: M1 , M8 , M16 , M17 , M20 , M42 , M43 .

  9. Supernova - Wikipedia

    en.wikipedia.org/wiki/Supernova

    The rate of mass loss for ... The 1054 supernova explosion that created the Crab Nebula in our galaxy had ... the emitted electromagnetic radiation is a tiny fraction ...