Institutional Repository of Radio Astronomy Research Laboratory
| 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
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| 2020-10-01 | |
| Source Publication | ASTROPHYSICAL JOURNAL LETTERS
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| ISSN | 2041-8205 |
| Volume | 902Issue:1Pages:L13 |
| Contribution Rank | 1 |
| 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 |
| URL | 查看原文 |
| Indexed By | SCI |
| Language | 英语 |
| WOS Keyword | GIANT PULSES ; SINGLE-PULSE ; RADIO PULSAR ; VARIABILITY ; SEARCH |
| Funding Project | National Key Research and Development Program of China[2016YFA0400804] ; National Key Research and Development Program of China[2017YFA0402600] ; Youth Innovation Promotion Association of Chinese Academy of Sciences ; CAS International Partnership Program[114A11KYSB20160008] ; 201* Project of Xinjiang Uygur Autonomous Region of China for Flexibly Fetching in Upscale Talents ; Strategic Priority Research Program (B) of the Chinese Academy of Sciences[XDB230102000] ; Operation, Maintenance and Upgrading Fund for Astronomical Telescopes and Facility Instruments from the Ministry of Finance of China (MOF) ; National Natural Science Foundation of China[11873080] ; Key Lab of FAST, National Astronomical Observatories, Chinese Academy of Sciences |
| WOS Research Area | Astronomy & Astrophysics |
| WOS Subject | Astronomy & Astrophysics |
| WOS ID | WOS:000577941100001 |
| Publisher | IOP PUBLISHING LTD |
| Funding Organization | National Key Research and Development Program of China ; Youth Innovation Promotion Association of Chinese Academy of Sciences ; CAS International Partnership Program ; 201* Project of Xinjiang Uygur Autonomous Region of China for Flexibly Fetching in Upscale Talents ; Strategic Priority Research Program (B) of the Chinese Academy of Sciences ; Operation, Maintenance and Upgrading Fund for Astronomical Telescopes and Facility Instruments from the Ministry of Finance of China (MOF) ; National Natural Science Foundation of China ; Key Lab of FAST, National Astronomical Observatories, Chinese Academy of Sciences |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://ir.xao.ac.cn/handle/45760611-7/3695 |
| Collection | 射电天文研究室_脉冲星研究团组 射电天文研究室 |
| Corresponding Author | Wang, J. B. |
| Affiliation | 1.Chinese Acad Sci, Xinjiang Astron Observ, 150 Sci 1 St, Urumqi 830011, Xinjiang, Peoples R China 2.Univ Chinese Acad Sci, Beijing 100049, Peoples R China 3.CSIRO Astron & Space Sci, POB 76, Epping, NSW 1710, Australia 4.Chinese Acad Sci, CAS Key Lab FAST, NAOC, Beijing 100101, Peoples R China 5.Chinese Acad Sci, Key Lab Radio Astron, 150 Sci 1 Str, Urumqi 830011, Xinjiang, Peoples R China 6.Xinjiang Key Lab Radio Astrophys, 150 Sci 1 Str, Urumqi 830011, Xinjiang, Peoples R China 7.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Peoples R China 8.Chinese Acad Sci, Natl Astron Observ, A20 Datun Rd, Beijing 100101, Peoples R China 9.Chinese Acad Sci, Natl Astron Observ, Key Lab Computat Astrophys, A20 Datun Rd, Beijing 100101, Peoples R China 10.Univ KwaZulu Natal, NAOC UKZN Computat Astrophys Ctr, ZA-4000 Durban, South Africa 11.Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China 12.Guizhou Normal Univ, Sch Phys & Elect Sci, Guiyang 550001, Peoples R China |
| First Author Affilication | Xinjiang Astronomical Observatory, Chinese Academy of Sciences |
| Corresponding Author Affilication | Xinjiang Astronomical Observatory, Chinese Academy of Sciences |
| Recommended Citation GB/T 7714 | Wang, S. Q.,Hobbs, G.,Wang, J. B.,et al. The Two Emission States of PSR B1534+12[J]. ASTROPHYSICAL JOURNAL LETTERS,2020,902(1):L13. |
| APA | Wang, S. Q..,Hobbs, G..,Wang, J. B..,Manchester, R..,Wang, N..,...&Zhang, L..(2020).The Two Emission States of PSR B1534+12.ASTROPHYSICAL JOURNAL LETTERS,902(1),L13. |
| MLA | Wang, S. Q.,et al."The Two Emission States of PSR B1534+12".ASTROPHYSICAL JOURNAL LETTERS 902.1(2020):L13. |
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| Wang-2020-The Two Em（1225KB） | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | View Application Full Text | |
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