Probing the Emission States of PSR J1107?5907
Wang,Jingbo1,2,3; Hobbs,George4,5; Kerr,Matthew6; Shannon,Ryan7,8; Dai,Shi4; Ravi,Vikram9; Cameron,Andrew4,5; Kaczmarek,Jane F.4; Hollow,Robert4; Li,Di5,10; Zhang,Lei4,5; Miao,Chenchen5; Yuan,Mao5; Wang,Shen5,11; Zhang,Songbo4,12; Xu,Heng5,13,14; Xu,Renxin13,14
Source PublicationThe Astrophysical Journal
AbstractAbstract The emission from PSR?J1107?5907 is erratic. Sometimes the radio pulse is undetectable, at other times the pulsed emission is weak, and for short durations the emission can be very bright. In order to improve our understanding of these state changes, we have identified archival data sets from the Parkes radio telescope in which the bright emission is present, and find that the emission never switches from the bright state to the weak state, but instead always transitions to the “off” state. Previous work had suggested the identification of the “off” state as an extreme manifestation of the weak state. However, the connection between the “off” and bright emission reported here suggests that the emission can be interpreted as undergoing only two emission states: a “bursting” state consisting of both bright pulses and nulls, and the weak emission state.
KeywordRadio pulsars Observational astronomy Astronomy data analysis
WOS IDIOP:0004-637X-889-1-ab5d38
PublisherThe American Astronomical Society
Citation statistics
Document Type期刊论文
Affiliation1.Xinjiang Astronomical Observatory, Chinese Academy of Sciences, 150 Science 1-Street, Urumqi, Xinjiang 830011, People's Republic of China;
2.Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, 150 Science 1-Street, Urumqi, Xinjiang, 830011, People's Republic of China
3.Xinjiang Key Laboratory of Radio Astrophysics, 150 Science 1-Street, Urumqi, Xinjiang, 830011, People's Republic of China
4.CSIRO Astronomy and Space Science, PO Box 76, Epping, NSW 1710, Australia
5.CAS Key Laboratory of FAST, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, People's Republic of China
6.Naval Research Laboratory, 4555 Overlook Ave., SW, Washington, DC 20375, USA
7.Centre for Astrophysics and Supercomputing, Swinburne University of Technology, P.O. Box 218, Hawthorn, Victoria 3122, Australia
8.ARC Centre of Excellence for Gravitational Wave Discovery (OzGrav), Hawthorn, Victoria, Australia
9.Cahill Center for Astronomy and Astrophysics, MC 249-17, California Institute of Technology, Pasadena, CA 91125, USA
10.NAOC-UKZN Computational Astrophysics Centre, University of KwaZulu-Natal, Durban 4000, South Africa
11.Astronomy Department, Cornell University, Ithaca, NY 14853, USA
12.Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, People's Republic of China
13.Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing 100871, People's Republic of China
14.Department of Astronomy, School of Physics, Peking University, Beijing 100871, People's Republic of China
Recommended Citation
GB/T 7714
Wang,Jingbo,Hobbs,George,Kerr,Matthew,et al. Probing the Emission States of PSR J1107?5907[J]. The Astrophysical Journal,2020,889(1).
APA Wang,Jingbo.,Hobbs,George.,Kerr,Matthew.,Shannon,Ryan.,Dai,Shi.,...&Xu,Renxin.(2020).Probing the Emission States of PSR J1107?5907.The Astrophysical Journal,889(1).
MLA Wang,Jingbo,et al."Probing the Emission States of PSR J1107?5907".The Astrophysical Journal 889.1(2020).
Files in This Item:
There are no files associated with this item.
Related Services
Recommend this item
Usage statistics
Export to Endnote
Google Scholar
Similar articles in Google Scholar
[Wang,Jingbo]'s Articles
[Hobbs,George]'s Articles
[Kerr,Matthew]'s Articles
Baidu academic
Similar articles in Baidu academic
[Wang,Jingbo]'s Articles
[Hobbs,George]'s Articles
[Kerr,Matthew]'s Articles
Bing Scholar
Similar articles in Bing Scholar
[Wang,Jingbo]'s Articles
[Hobbs,George]'s Articles
[Kerr,Matthew]'s Articles
Terms of Use
No data!
Social Bookmark/Share
All comments (0)
No comment.

Items in the repository are protected by copyright, with all rights reserved, unless otherwise indicated.