We present the results of two-frequency flux density measurements of 74 pulsars with the Culgoora circular array. We show that the spectral index of a typical pulsar steepens markedly from 80 to 1400 MHz, but we found no significant relationship between the metre-wave spectral index and the published pulsar parameters
CITATION STYLE
Slee, O., Alurkar, S., & Bobra, A. (1986). Flux Densities, Spectra and Variability of Pulsars at Metre Wavelengths. Australian Journal of Physics, 39(1), 103. https://doi.org/10.1071/ph860103
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