Detection of decametre-wavelength pulsed radio emission of 40 known pulsars

The study of pulsars at the lowest radio frequencies observable from the ground (10-30 MHz) is complicated by strong interstellar (dispersion, scattering) and ionospheric (scintillation, refraction) propagation effects, as well as intense Galactic background noise and interference. However, it permi...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2013-06, Vol.431 (4), p.3624-3641
Hauptverfasser:	Zakharenko, V. V., Vasylieva, I. Y., Konovalenko, A. A., Ulyanov, O. M., Serylak, M., Zarka, P., Grießmeier, J.-M., Cognard, I., Nikolaenko, V. S.
Format:	Artikel
Sprache:	eng
Schlagworte:	Pulsars Radio astronomy Sciences of the Universe Space telescopes Stars & galaxies
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