Nearly every wavelength is emitted by this object's central (*) pulsar, whose interactions with fast electrons are thought to produce its central blue region through synchrotron radiation, as proposed by Iosif Shklovsky.
Mori et al demonstrated the spatial variation of this object's spectrum, with photon indices of 1.9 within a central torus and 3.0 at its periphery, while the axis along its jet demonstrates photon indices of 2.0 to 2.5. Slipher found that its spectral lines are split due to redshift, and this object may have four magnetic poles rather than the more typical two, which could explain irregular secondary bursts of energy. Nearly every wavelength is emitted by this object's central (*) pulsar, whose interactions with fast electrons are thought to produce its central blue region through synchrotron radiation, as proposed by Iosif Shklovsky. Â For 10 points name this remnant of a supernova, a nebula which comprises part of Taurus and is designated M1.
Mori et al demonstrated the spatial variation of this object's spectrum, with photon indices of 1.9 within a central torus and 3.0 at its periphery, while the axis along its jet demonstrates photon indices of 2.0 to 2.5.
Crab Nebula