KMS National Astronomical Observatories, CAS
| The Two Emission States of PSR B1534+12 | |
| Wang,S. Q.1,2,3,4; Hobbs,G.3; Wang,J. B.1,5,6; Manchester,R.3; Wang,N.1,5,6; Zhang,S. B.2,3,7; Feng,Y.2,3,8; Wang,W.-Y.2,9; Li,D.2,8,10; Dai,S.3; Lee,K. J.11; Dang,S. J.1,2,12; Zhang,L.2,3,8 | |
| 2020-10-01 | |
| Source Publication | The Astrophysical Journal Letters
 |
| ISSN | 2041-8205 |
| Volume | 902Issue:1 |
| Abstract | Abstract We have observed PSR?B1534+12 (J1537+1155), a pulsar with a neutron star companion, using the Five-hundred-meter Aperture Spherical radio Telescope. We found that this pulsar shows two distinct emission states: a weak state with a wide pulse profile and a burst state with a narrow pulse profile. The weak state is always present. We cannot, with our current data, determine whether the pulse energy of the weak state follows a normal or a log-normal distribution. The burst state energy distribution follows a power law. The amplitude of the single-pulse emission in the burst state varies significantly; the peak flux intensity of the brightest pulse is 334 times stronger than that of the average pulse. We also examined the timing precision achievable using only bright pulses, which showed no demonstrable improvement because of pulse jitter and therefore quantified the jitter noise level for this pulsar. |
| Keyword | Millisecond pulsars Radio pulsars Astronomy data analysis |
| DOI | 10.3847/2041-8213/abbb89 |
| Language | 英语 |
| WOS ID | IOP:2041-8205-902-1-abbb89 |
| Publisher | The American Astronomical Society |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://ir.bao.ac.cn/handle/114a11/57654 |
| Collection | 中国科学院国家天文台 |
| Affiliation | 1.Xinjiang Astronomical Observatory, Chinese Academy of Sciences, 150 Science 1-Street, Urumqi, Xinjiang 830011, People's Republic of China; wangjingbo@xao.ac.cn 2.University of Chinese Academy of Sciences, Beijing 100049, People's Republic of China 3.CSIRO Astronomy and Space Science, P.O. Box 76, Epping, NSW 1710, Australia 4.CAS Key Laboratory of FAST, NAOC, Chinese Academy of Sciences, Beijing 100101, People’s Republic of China 5.Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, 150 Science 1-Street, Urumqi, Xinjiang, 830011, People's Republic of China 6.Xinjiang Key Laboratory of Radio Astrophysics, 150 Science1-Street, Urumqi, Xinjiang, 830011, People's Republic of China 7.Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, People's Republic of China 8.National Astronomical Observatories, Chinese Academy of Sciences, A20 Datun Road, Chaoyang District, Beijing 100101, People's Republic of China 9.Key Laboratory for Computational Astrophysics, National Astronomical Observatories, Chinese Academy of Sciences, 20A Datun Road, Beijing 100101, People's Republic of China 10.NAOC-UKZN Computational Astrophysics Centre, University of KwaZulu-Natal, Durban 4000, South Africa 11.Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing 100871, People's Republic of China 12.School of Physics and Electronic Science, Guizhou Normal University, Guiyang, 550001, People's Republic of China |
| Recommended Citation GB/T 7714 | Wang,S. Q.,Hobbs,G.,Wang,J. B.,et al. The Two Emission States of PSR B1534+12[J]. The Astrophysical Journal Letters,2020,902(1). |
| APA | Wang,S. Q..,Hobbs,G..,Wang,J. B..,Manchester,R..,Wang,N..,...&Zhang,L..(2020).The Two Emission States of PSR B1534+12.The Astrophysical Journal Letters,902(1). |
| MLA | Wang,S. Q.,et al."The Two Emission States of PSR B1534+12".The Astrophysical Journal Letters 902.1(2020). |
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