The Study for Mode Changing for Radio Pulsar <scp>J0742</scp>‐2822 at 3.1 GHz

ABSTRACT The mode switching of PSR J0742‐2822 at 3.1 GHz was investigated using single‐pulse data from the Parkes 64‐m radio telescope in Australia. By analyzing the ratio of the relative intensity of the two components for each sub‐integral profile, we classified the integral profile of this source into two modes: normal mode and abnormal mode. We then obtained the average profile of PSR J0742‐2822 at 3.1 GHz for each mode. The results indicate that the normal and abnormal modes of integrated pulse profiles occurred 72% and 28% of the time, respectively, over a total of 3.7 h of observation. This study is significant for understanding the theoretical mechanism behind the pulsar mode‐switching phenomenon.

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Publication Details

Journal
Astronomische Nachrichten
Published
2025-03-08
DOI
https://doi.org/10.1002/asna.20250032
Primary Topic
Pulsars and Gravitational Waves Research
Type
article
Field-Weighted Citation Impact
0.00

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article

The Study for Mode Changing for Radio Pulsar J0742‐2822 at 3.1 GHz

Jun Tan, Jinpeng Wang, Jia‐Wei Wang, Cheng‐Bing Lyu et al.
Astronomische Nachrichten
Pulsars and Gravitational Waves Research
article

The Study for Mode Changing for Radio Pulsar J0742‐2822 at 3.1 GHz

Jun Tan, Jinpeng Wang, Jia‐Wei Wang, Cheng‐Bing Lyu, Hui Wang
article en

Abstract

ABSTRACT The mode switching of PSR J0742‐2822 at 3.1 GHz was investigated using single‐pulse data from the Parkes 64‐m radio telescope in Australia. By analyzing the ratio of the relative intensity of the two components for each sub‐integral profile, we classified the integral profile of this source into two modes: normal mode and abnormal mode. We then obtained the average profile of PSR J0742‐2822 at 3.1 GHz for each mode. The results indicate that the normal and abnormal modes of integrated pulse profiles occurred 72% and 28% of the time, respectively, over a total of 3.7 h of observation. This study is significant for understanding the theoretical mechanism behind the pulsar mode‐switching phenomenon.

Astronomische NachrichtenVol. 346(7-8)
Yuncheng University (CN), Guangzhou University (CN), Guilin University of Technology (CN)
National Natural Science Foundation of China, Natural Science Foundation of Shanxi Province
Openalex Percentile: Top 97%
Pulsars and Gravitational Waves Research
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