PSR J1926-0652: A Pulsar with Interesting Emission Properties Discovered at FAST. (arXiv:1904.05482v1 [astro-ph.HE])

PSR J1926-0652: A Pulsar with Interesting Emission Properties Discovered at FAST. (arXiv:1904.05482v1 [astro-ph.HE])
<a href="http://arxiv.org/find/astro-ph/1/au:+Zhang_L/0/1/0/all/0/1">Lei Zhang</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Li_D/0/1/0/all/0/1">Di Li</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Hobbs_G/0/1/0/all/0/1">George Hobbs</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Agar_C/0/1/0/all/0/1">Crispin H. Agar</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Manchester_R/0/1/0/all/0/1">Richard N. Manchester</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Weltevrede_P/0/1/0/all/0/1">Patrick Weltevrede</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Coles_W/0/1/0/all/0/1">William A. Coles</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Wang_P/0/1/0/all/0/1">Pei Wang</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Zhu_W/0/1/0/all/0/1">Weiwei Zhu</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Wen_Z/0/1/0/all/0/1">Zhigang Wen</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Yuan_J/0/1/0/all/0/1">Jianping Yuan</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Cameron_A/0/1/0/all/0/1">Andrew D. Cameron</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Dai_S/0/1/0/all/0/1">Shi Dai</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Liu_K/0/1/0/all/0/1">Kuo Liu</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Zhi_Q/0/1/0/all/0/1">Qijun Zhi</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Miao_C/0/1/0/all/0/1">Chenchen Miao</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Yua_M/0/1/0/all/0/1">Mao Yua</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Cao_S/0/1/0/all/0/1">Shuyun Cao</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Feng_L/0/1/0/all/0/1">Li Feng</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Gan_H/0/1/0/all/0/1">Hengqian Gan</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Gao_L/0/1/0/all/0/1">Long Gao</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Gu_X/0/1/0/all/0/1">Xuedong Gu</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Guo_M/0/1/0/all/0/1">Minglei Guo</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Hao_Q/0/1/0/all/0/1">Qiaoli Hao</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Huang_L/0/1/0/all/0/1">Lin Huang</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Jiang_P/0/1/0/all/0/1">Peng Jiang</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Jin_C/0/1/0/all/0/1">Chengjin Jin</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Li_H/0/1/0/all/0/1">Hui Li</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Li_Q/0/1/0/all/0/1">Qi Li</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Li_Q/0/1/0/all/0/1">Qisheng Li</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Liu_H/0/1/0/all/0/1">Hongfei Liu</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Pan_G/0/1/0/all/0/1">Gaofeng Pan</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Pan_Z/0/1/0/all/0/1">Zhichen Pan</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Peng_B/0/1/0/all/0/1">Bo Peng</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Qian_H/0/1/0/all/0/1">Hui Qian</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Qian_L/0/1/0/all/0/1">Lei Qian</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Shi_X/0/1/0/all/0/1">Xiangwei Shi</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Song_J/0/1/0/all/0/1">Jinyou Song</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Song_L/0/1/0/all/0/1">Liqiang Song</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Sun_C/0/1/0/all/0/1">Caihong Sun</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Sun_J/0/1/0/all/0/1">Jinghai Sun</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Wang_H/0/1/0/all/0/1">Hong Wang</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Wang_Q/0/1/0/all/0/1">Qiming Wang</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Wang_Y/0/1/0/all/0/1">Yi Wang</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Xie_X/0/1/0/all/0/1">Xiaoyao Xie</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Yan_J/0/1/0/all/0/1">Jun Yan</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Yang_L/0/1/0/all/0/1">Li Yang</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Yang_S/0/1/0/all/0/1">Shimo Yang</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Yao_R/0/1/0/all/0/1">Rui Yao</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Yu_D/0/1/0/all/0/1">Dongjun Yu</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Yu_J/0/1/0/all/0/1">Jinglong Yu</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Yue_Y/0/1/0/all/0/1">Youling Yue</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Zhang_C/0/1/0/all/0/1">Chengmin Zhang</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Zhang_H/0/1/0/all/0/1">Haiyan Zhang</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Zhang_S/0/1/0/all/0/1">Shuxin Zhang</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Zheng_X/0/1/0/all/0/1">Xiaonian Zheng</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Zhou_A/0/1/0/all/0/1">Aiying Zhou</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Zhu_B/0/1/0/all/0/1">Boqin Zhu</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Zhu_L/0/1/0/all/0/1">Lichun Zhu</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Zhu_M/0/1/0/all/0/1">Ming Zhu</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Zhu_W/0/1/0/all/0/1">Wenbai Zhu</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Zhu_Y/0/1/0/all/0/1">Yan Zhu</a>

We describe PSR J1926-0652, a pulsar recently discovered with the
Five-hundred-meter Aperture Spherical radio Telescope (FAST). Using sensitive
single-pulse detections from FAST and long-term timing observations from the
Parkes 64-m radio telescope, we probed phenomena on both long and short time
scales. The FAST observations covered a wide frequency range from 270 to 800
MHz, enabling individual pulses to be studied in detail. The pulsar exhibits at
least four profile components, short-term nulling lasting from 4 to 450 pulses,
complex subpulse drifting behaviours and intermittency on scales of tens of
minutes. While the average band spacing P3 is relatively constant across
different bursts and components, significant variations in the separation of
adjacent bands are seen, especially near the beginning and end of a burst. Band
shapes and slopes are quite variable, especially for the trailing components
and for the shorter bursts. We show that for each burst the last detectable
pulse prior to emission ceasing has different properties compared to other
pulses. These complexities pose challenges for the classic carousel-type
models.

http://arxiv.org/icons/sfx.gif