Research articles

search articles

My Pages

Stat

Members: 3645
Articles: 2'504'928
Articles rated: 2609

25 April 2024

» arxiv » 1904.5482

Article overview

PSR J1926-0652: A Pulsar with Interesting Emission Properties Discovered at FAST
Lei Zhang ; Di Li ; George Hobbs ; Crispin H. Agar ; Richard N. Manchester ; Patrick Weltevrede ; William A. Coles ; Pei Wang ; Weiwei Zhu ; Zhigang Wen ; Jianping Yuan ; Andrew D. Cameron ; Shi Dai ; Kuo Liu ; Qijun Zhi ; Chenchen Miao ; Mao Yua ; Shuyun Cao ; Li Feng ; Hengqian Gan ; Long Gao ; Xuedong Gu ; Minglei Guo ; Qiaoli Hao ; Lin Huang ; Peng Jiang ; Chengjin Jin ; Hui Li ; Qi Li ; Qisheng Li ; Hongfei Liu ; Gaofeng Pan ; Zhichen Pan ; Bo Peng ; Hui Qian ; Lei Qian ; Xiangwei Shi ; Jinyou Song ; Liqiang Song ; Caihong Sun ; Jinghai Sun ; Hong Wang ; Qiming Wang ; Yi Wang ; Xiaoyao Xie ; Jun Yan ; Li Yang ; Shimo Yang ; Rui Yao ; Dongjun Yu ; Jinglong Yu ; Youling Yue ; Chengmin Zhang ; Haiyan Zhang ; Shuxin Zhang ; Xiaonian Zheng ; Aiying Zhou ; Boqin Zhu ; Lichun Zhu ; Ming Zhu ; Wenbai Zhu ; Yan Zhu ;
Date:	11 Apr 2019
Abstract:	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.
Source:	arXiv, 1904.5482
Services:	Forum \| Review \| PDF \| Favorites

No review found.

Did you like this article?

This article or document is ...
important:
of broad interest:
readable:
new:
correct:
Global appreciation:

Note: answers to reviews or questions about the article must be posted in the forum section.
Authors are not allowed to review their own article. They can use the forum section.

browser Mozilla/5.0 AppleWebKit/537.36 (KHTML, like Gecko; compatible; ClaudeBot/1.0; +claudebot@anthropic.com)

ScienXe.org
» my Online CV
» Free

News, job offers and information for researchers and scientists:

home

contact

sitemap