Recent arguments supporting a suggestion to observe pulsars via their direct mode of magnetic-dipole radiation

Physics

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Magnetic Dipoles, Pulsars, Stellar Radiation, Binary Stars, Signal Processing, Stellar Evolution

Scientific paper

The detection of pulsars by their direct-mode magnetic-dipole radiation (proposed by Kaplan, 1972 and 1974) is discussed in the light of the discovery of the 1.5-msec (642-Hz) pulsar by Backer et al. (1982) and Baker (1982). The existence of numerous pulsars with frequencies in the 1-kHz range is predicted, ad the analysis of archived data from NASA outer-solar-system probes is suggested as a useful method for discovering new objects via direct-mode radiation. Pulsar models relating the observations to evolutionary stages of binary formation are briefly characterized.

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