Periodic Q-mode modulation in PSR J1825-0935 (PSR B1822-09) | |
Yan, W. M.2,3; Manchester, R. N.4; Wang, N.2,3,5; Yuan, J. P.2,3,5; Wen, Z. G.2,3; Lee, K. J.1,6 | |
刊名 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
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2019-05-01 | |
卷号 | 485期号:3页码:3242-+ |
关键词 | stars: neutron pulsars: general pulsars: individual (PSR J1825-0935) |
ISSN号 | 0035-8711 |
DOI | 10.1093/mnras/stz650 |
英文摘要 | PSR J1825-0935 (PSR B1822-09) switches between radio-quiet (Q-mode) and radio-bright (B-mode) modes. The Q-mode is known to have a periodic fluctuation that modulates both the interpulse and the main pulse with the same period. Earlier investigators argued that the periodic Q-mode modulation is associated with drifting subpulses. We report on single-pulse observations of PSR J1825-0935 that were made using the Parkes 64-m radio telescope with a central frequency of 1369 MHz. The high-sensitivity observations revealed that the periodic Q-mode modulation is in fact a periodic longitude-stationary intensity modulation occurring in the interpulse and the main pulse. The fluctuation spectral analysis showed that the modulation period is about 43P1, where P1 is the rotation period of the pulsar. Furthermore, we confirm that themodulation patterns in the interpulse and themain pulse are phase-locked. Specifically, the intensities of the interpulse and the immediately following main pulse are more highly correlated than for the main pulse and interpulse at any other lag. Polarization properties of the strong and weak Q-mode states are different, even for the trailing part of the main pulse which does not show the periodic intensity modulation. |
资助项目 | National Basic Research Program of China (973 Program)[2015CB857100] ; National Natural Science Foundation of China[U1831102] ; National Natural Science Foundation of China[U1731238] ; National Natural Science Foundation of China[U1631106] ; National Natural Science Foundation of China[11873080] ; National Natural Science Foundation of China[U1838109] ; Strategic Priority Research Program of Chinese Academy of Sciences[XDB23010200] ; National Key Research and Development Program of China[2016YFA0400800] ; 2016 Project of Xinjiang Uygur Autonomous Region of China for Flexibly Fetching in Upscale Talents ; CAS 'Light of West China' Program[2016-QNXZ-B-24] ; CAS 'Light of West China' Program[2017-XBQNXZ-B-022] ; Commonwealth of Australia |
WOS关键词 | DYNAMIC EMISSION PROPERTIES ; INTERPULSE INTERACTION ; GLITCH ACTIVITY ; RADIO-EMISSION ; PULSAR ; NULLS ; DISCOVERY ; PSRCHIVE ; PSRFITS |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
出版者 | OXFORD UNIV PRESS |
WOS记录号 | WOS:000474902000019 |
资助机构 | National Basic Research Program of China (973 Program) ; National Basic Research Program of China (973 Program) ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Strategic Priority Research Program of Chinese Academy of Sciences ; Strategic Priority Research Program of Chinese Academy of Sciences ; National Key Research and Development Program of China ; National Key Research and Development Program of China ; 2016 Project of Xinjiang Uygur Autonomous Region of China for Flexibly Fetching in Upscale Talents ; 2016 Project of Xinjiang Uygur Autonomous Region of China for Flexibly Fetching in Upscale Talents ; CAS 'Light of West China' Program ; CAS 'Light of West China' Program ; Commonwealth of Australia ; Commonwealth of Australia ; National Basic Research Program of China (973 Program) ; National Basic Research Program of China (973 Program) ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Strategic Priority Research Program of Chinese Academy of Sciences ; Strategic Priority Research Program of Chinese Academy of Sciences ; National Key Research and Development Program of China ; National Key Research and Development Program of China ; 2016 Project of Xinjiang Uygur Autonomous Region of China for Flexibly Fetching in Upscale Talents ; 2016 Project of Xinjiang Uygur Autonomous Region of China for Flexibly Fetching in Upscale Talents ; CAS 'Light of West China' Program ; CAS 'Light of West China' Program ; Commonwealth of Australia ; Commonwealth of Australia ; National Basic Research Program of China (973 Program) ; National Basic Research Program of China (973 Program) ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Strategic Priority Research Program of Chinese Academy of Sciences ; Strategic Priority Research Program of Chinese Academy of Sciences ; National Key Research and Development Program of China ; National Key Research and Development Program of China ; 2016 Project of Xinjiang Uygur Autonomous Region of China for Flexibly Fetching in Upscale Talents ; 2016 Project of Xinjiang Uygur Autonomous Region of China for Flexibly Fetching in Upscale Talents ; CAS 'Light of West China' Program ; CAS 'Light of West China' Program ; Commonwealth of Australia ; Commonwealth of Australia ; National Basic Research Program of China (973 Program) ; National Basic Research Program of China (973 Program) ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Strategic Priority Research Program of Chinese Academy of Sciences ; Strategic Priority Research Program of Chinese Academy of Sciences ; National Key Research and Development Program of China ; National Key Research and Development Program of China ; 2016 Project of Xinjiang Uygur Autonomous Region of China for Flexibly Fetching in Upscale Talents ; 2016 Project of Xinjiang Uygur Autonomous Region of China for Flexibly Fetching in Upscale Talents ; CAS 'Light of West China' Program ; CAS 'Light of West China' Program ; Commonwealth of Australia ; Commonwealth of Australia |
内容类型 | 期刊论文 |
源URL | [http://ir.bao.ac.cn/handle/114a11/26897] ![]() |
专题 | 中国科学院国家天文台 |
通讯作者 | Yan, W. M. |
作者单位 | 1.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China 2.Chinese Acad Sci, Xinjiang Astron Observ, 150 Sci 1 St, Urumqi 830011, Xinjiang, Peoples R China 3.Chinese Acad Sci, Key Lab Radio Astron, Nanjing 210008, Jiangsu, Peoples R China 4.Australia Telescope Natl Facil, CSIRO Astron & Space Sci, POB 76, Epping, NSW 1710, Australia 5.Xinjiang Key Lab Radio Astrophys, 150 Sci 1 St, Urumqi 830011, Xinjiang, Peoples R China 6.Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China |
推荐引用方式 GB/T 7714 | Yan, W. M.,Manchester, R. N.,Wang, N.,et al. Periodic Q-mode modulation in PSR J1825-0935 (PSR B1822-09)[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2019,485(3):3242-+. |
APA | Yan, W. M.,Manchester, R. N.,Wang, N.,Yuan, J. P.,Wen, Z. G.,&Lee, K. J..(2019).Periodic Q-mode modulation in PSR J1825-0935 (PSR B1822-09).MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,485(3),3242-+. |
MLA | Yan, W. M.,et al."Periodic Q-mode modulation in PSR J1825-0935 (PSR B1822-09)".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 485.3(2019):3242-+. |
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