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arXiv · 1206.5885

A study of strong pulses detected from PSR B0656+14 using Urumqi 25-m radio telescope at 1540MHz

Guo-Cun Tao·Ali Esamdin·Hui-Dong Hu·Mao-Fei Qian·Jing Li·Na Wang
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Abstract

We report on the properties of strong pulses from PSR B0656+14 by analyzing the data obtained using Urumqi 25-m radio telescope at 1540 MHz from August 2007 to September 2010. In 44 hrs of observational data, a total of 67 pulses with signal-to-noise ratios above a 5-{\sigma} threshold were detected. The peak flux densities of these pulses are 58 to 194 times that of the average profile, and the pulse energies of them are 3 to 68 times that of the average pulse. These pulses are clustered around phases about 5 degrees ahead of the peak of the average profile. Comparing with the width of the average profile, they are relatively narrow, with the full widths at half-maximum range from 0.28 to 1.78 degrees. The distribution of pulse-energies of the pulses follows a lognormal distribution. These sporadic strong pulses detected from PSR B0656+14 are different in character from the typical giant pulses, and from its regular pulses.

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Guo-Cun Tao, Ali Esamdin, Hui-Dong Hu, Mao-Fei Qian, Jing Li, Na Wang. 2012-06-26. A study of strong pulses detected from PSR B0656+14 using Urumqi 25-m radio telescope at 1540MHz. https://doi.org/10.1088/1674-4527/12/12/006

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