Special relativistic simulations predict detectable radio emission from nightside magnetic structures around planets in pulsar winds, including for the known planet PSR J0636+5129 b.
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Timing solutions and basic properties are presented for two new pulsars, PSR J0535-0231 (415 ms, likely disrupted recycled) and PSR J1816-0518 (1.93 s), with noted shortfalls in NE2001 and YMW16 electron density models for the first.
Coherent timing solutions at 150 MHz for 17 pulsars from Irish LOFAR observations, including 7 without prior solutions.
citing papers explorer
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Planets in Pulsar Winds
Special relativistic simulations predict detectable radio emission from nightside magnetic structures around planets in pulsar winds, including for the known planet PSR J0636+5129 b.
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Discovery and Timing Follow-Up of Two FAST-Discovered Pulsars from the FAST CRAFTS Survey
Timing solutions and basic properties are presented for two new pulsars, PSR J0535-0231 (415 ms, likely disrupted recycled) and PSR J1816-0518 (1.93 s), with noted shortfalls in NE2001 and YMW16 electron density models for the first.
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Pulsar timing solutions for 17 pulsars at 150 MHz from the Irish LOFAR station
Coherent timing solutions at 150 MHz for 17 pulsars from Irish LOFAR observations, including 7 without prior solutions.