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  2. Crab Nebula - Wikipedia

    en.wikipedia.org/wiki/Crab_Nebula

    The Crab Nebula (catalogue designations M1, NGC 1952, Taurus A) is a supernova remnant and pulsar wind nebula in the constellation of Taurus. The common name comes from a drawing that somewhat resembled a crab with arms produced by William Parsons, 3rd Earl of Rosse , in 1842 or 1843 using a 36-inch (91 cm) telescope . [ 6 ]

  3. Pulsar - Wikipedia

    en.wikipedia.org/wiki/Pulsar

    The Crab pulsar 33-millisecond pulse period was too short to be consistent with other proposed models for pulsar emission. Moreover, the Crab pulsar is so named because it is located at the center of the Crab Nebula, consistent with the 1933 prediction of Baade and Zwicky. [ 23 ]

  4. Pulsar wind nebula - Wikipedia

    en.wikipedia.org/wiki/Pulsar_wind_nebula

    A pulsar wind nebula (PWN, plural PWNe), sometimes called a plerion (derived from the Greek "πλήρης", pleres, meaning "full"), [1] is a type of nebula sometimes found inside the shell of a supernova remnant (SNR), powered by winds generated by a central pulsar.

  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.

  6. Crab Pulsar - Wikipedia

    en.wikipedia.org/wiki/Crab_Pulsar

    Thomas Gold has shown that the pulsar's spin-down power is sufficient to power the Crab Nebula. A subsequent study by them, including William D. Brundage, also found that the NP 0532 source is located at the Crab Nebula. [20] A radio source was also reported coincident with the Crab Nebula in late 1968 by L. I. Matveenko in Soviet Astronomy. [21]

  7. Supernova - Wikipedia

    en.wikipedia.org/wiki/Supernova

    The pulsar in the Crab Nebula is travelling at 375 km/s relative to the nebula. [ 165 ] A long-standing puzzle surrounding type II supernovae is why the remaining compact object receives a large velocity away from the epicentre; [ 166 ] pulsars , and thus neutron stars, are observed to have high peculiar velocities , and black holes presumably ...

  8. Period-luminosity relation - Wikipedia

    en.wikipedia.org/wiki/Period-luminosity_relation

    In astronomy, a period-luminosity relation is a relationship linking the luminosity of pulsating variable stars with their pulsation period. The best-known relation is the direct proportionality law holding for Classical Cepheid variables , sometimes called the Leavitt Law .

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