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Wide-bandwidth Observations of PSR J0941–39 and PSR J1107–5907
Sun,S. N.1,2; Wang,N.1,2,3; Yan,W. M.1,2,3; Wang,S. Q.1,2; Xie,J. T.4
2023-12-01
Source PublicationThe Astrophysical Journal
ISSN0004-637X
Volume959Issue:1Pages:56
Contribution Rank1
AbstractAbstract We present a polarization analysis of PSR J0941–39 and PSR J1107–5907, which exhibit transitions between being pulsars and rotating radio transients (RRATs), using the ultrawide-bandwidth low-frequency receiver on Murriyang, the Parkes 64 m radio telescope. The spectral index of each pulsar was measured, revealing distinct variations among different states. By using the rotating vector model, we determined that the geometry of the magnetosphere remains consistent between the RRAT state and the pulsar state for PSR J0941–39, with emissions originating from the same height in the magnetosphere. The occurrence of the RRAT state could be attributed to variations in currents within the pulsar’s magnetosphere. Our results suggest that the emission mechanism of an RRAT may share similarities with that of a typical pulsar.
KeywordPulsars Radio pulsars Astrophysics - High Energy Astrophysical Phenomena
DOI10.3847/1538-4357/ad0a8e
Indexed BySCI
Language英语
WOS IDWOS:001116866200001
PublisherThe American Astronomical Society
Citation statistics
Cited Times:1[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/6351
Collection中国科学院新疆天文台
Corresponding AuthorWang,N.
Affiliation1.Xinjiang Astronomical Observatory, Chinese Academy of Sciences, Urumqi, Xinjiang 830011, People’s Republic of China; na.wang@xao.ac.cn
2.Xinjiang Key Laboratory of Radio Astrophysics, 150 Science1-Street, Urumqi 830011, People’s Republic of China
3.Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, Nanjing 210008, People’s Republic of China
4.Research Center for Intelligent Computing Platforms, Zhejiang Laboratory, Hangzhou 311100, People’s Republic of China
First Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Corresponding Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Sun,S. N.,Wang,N.,Yan,W. M.,等. Wide-bandwidth Observations of PSR J0941–39 and PSR J1107–5907[J]. The Astrophysical Journal,2023,959(1):56.
APA Sun,S. N.,Wang,N.,Yan,W. M.,Wang,S. Q.,&Xie,J. T..(2023).Wide-bandwidth Observations of PSR J0941–39 and PSR J1107–5907.The Astrophysical Journal,959(1),56.
MLA Sun,S. N.,et al."Wide-bandwidth Observations of PSR J0941–39 and PSR J1107–5907".The Astrophysical Journal 959.1(2023):56.
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