Low Mode Coherent Synchrotron Radiation and Pulsar Phenomena

@article{Eastlund1970LowMC,
  title={Low Mode Coherent Synchrotron Radiation and Pulsar Phenomena},
  author={Bernard J. Eastlund},
  journal={Nature},
  year={1970},
  volume={225},
  pages={430-434}
}
Information on the properties and distributions of the charges responsible for pulsar emission can be deduced from an appraisal of the coherent synchrotron radiation from an oblique rotator model. 

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Theory of pulsar magnetospheres

There is a wide range of fundamental physical problems directly related to how pulsars function. Some of these are independent of the specific pulsar mechanism. Others relate directly to the physics

The crab nebula

The nature of radio emission from pulsars

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Stars with a dipole magnetic field oriented at an angle to the rotation axis may emit pulsating radio signals.

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THE observation that the pulsar CP 0328 radiates single pulses which seem to be basic elements of the total radio radiation, and which are highly polarized1, led at first to the suggestion that the

Observations of Pulsar NP 0527

SINCE December 20, 1968, we have observed a pulsar in the vicinity of the Crab Nebula with the longest period yet reported for any pulsar. Measurements have been made with the 1,000 foot diameter

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Some Difficulties with the Oblique Rotator Model for Pulsars

PRACTICALLY all the available evidence up to now (short duration of pulses, rapid pulsing, slowing down of the period, association with past supernovae, and so on) suggests that pulsars are produced

Magnetic Dipole Radiation from Pulsars

RADIO astronomers1–3 have recently discovered pulsars in Vela and near the Crab nebula which seem to be associated with supernova remnants and have repetition periods (0.0892 s and 0.0331 s)

Population II Star Models and Abundance of Primaeval Helium

SINCE the discovery of the 3° K cosmic blackbody radiation1, the hypothesis of helium formation in a primordial fireball has received some support. Peebles2 and Wagoner, Fowler and Hoyle3 have