Monitoring of the radio emission of the Crab Nebula pulsar at low frequencies
Results of long-term (2002–2010) monitoring of giant radio pulses of the pulsar PSR B0531+21 in the Crab Nebula at ν = 44, 63, and 111 MHz are reported. The observations were conducted on the LPA and DKR-1000 radio telescopes of the Lebedev Physical Institute. The giant pulses were analyzed using sp...
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Veröffentlicht in: | Astronomy reports 2011-05, Vol.55 (5), p.416-424 |
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Sprache: | eng |
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