Radio Emission Variability of Supernova Remnants and a Possible Explanation of the Phenomenon

The flux densities and current spectra of plerions and combined supernova remnants (SNRs): 3C58, 3C144, G11.2–0.3, G21.5–0.9, and 3C396 are determined on an artificial moon (AM) flux scale. The radio emission variability of the objects on different time scales is studied by multiple measurements usi...

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Veröffentlicht in:	Astronomy reports 2022-11, Vol.66 (11), p.953-964
Hauptverfasser:	Ivanov, V. P., Ipatov, A. V., Rakhimov, I. A., Andreeva, T. S.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy Emission analysis Fluctuations Observations and Techniques Physics Physics and Astronomy Radio emission Radio telescopes Solar flares Supernova Supernova remnants
Online-Zugang:	Volltext
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