Discovery of gamma-Ray Pulsations from PSR J1835-3259B in the Globular Cluster NGC 6652
文献类型：期刊论文
| 作者 | Zhang, Pengfei1; Xing, Yi2; Wang, Zhongxiang1,2 |
| 刊名 | ASTROPHYSICAL JOURNAL LETTERS
 |
| 出版日期 | 2022-08-01 |
| 卷号 | 935期号:2页码:4 |
| ISSN号 | 2041-8205 |
| DOI | 10.3847/2041-8213/ac88bf |
| 英文摘要 | Motivated by the recent discovery of the pulsar J1835-3259B with a spin period 1.83 ms in the globular cluster (GC) NGC 6652, we analyze the gamma-ray data obtained with the Large Area Telescope on board the Fermi Gamma-ray Space Telescope (Fermi) for the GC and detect the pulsations of this millisecond pulsar (MSP) at a 5.4 sigma confidence level (the weighted H-test value is similar to 41). From timing analysis of the data, a pulse profile that is similar to the radio one is established. We thus consider that we have detected the gamma-ray emission of the MSP, and discuss the implications. Based on the results of our analysis and different studies of the sources in the GC, the observed gamma-ray emission from the GC could mainly arise from this MSP, like the previous two cases in the GCs NGC 6624 and NGC 6626. Assuming this is the case, the pulsar, at the GC's distance of 9.46 kpc and having a spin-down luminosity of <= 4.3 x 10(35) erg s(-1), would have a gamma-ray luminosity of similar or equal to(5.04 +/- 0.44) x 10(34) erg s(-1) and a gamma-ray efficiency of greater than or similar to 0.12. |
| WOS关键词 | LARGE-AREA TELESCOPE ; TRANSITIONAL MILLISECOND PULSAR ; EMISSION ; EVOLUTION ; CATALOG |
| 资助项目 | National Key R&D Program of China[2018YFA0404204] ; National Natural Science Foundation of China[12163006] ; Basic Research Program of Yunnan Province[202201AS070005] ; Basic Research Program of Yunnan Province[202201AT070137] ; Foundations of Yunnan Province[202201BF070001-020] ; Original Innovation Program of the Chinese Academy of Sciences[E085021002] |
| WOS研究方向 | Astronomy & Astrophysics |
| 语种 | 英语 |
| WOS记录号 | WOS:000843294300001 |
| 出版者 | IOP Publishing Ltd |
| 资助机构 | National Key R&D Program of China ; National Key R&D Program of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Basic Research Program of Yunnan Province ; Basic Research Program of Yunnan Province ; Foundations of Yunnan Province ; Foundations of Yunnan Province ; Original Innovation Program of the Chinese Academy of Sciences ; Original Innovation Program of the Chinese Academy of Sciences ; National Key R&D Program of China ; National Key R&D Program of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Basic Research Program of Yunnan Province ; Basic Research Program of Yunnan Province ; Foundations of Yunnan Province ; Foundations of Yunnan Province ; Original Innovation Program of the Chinese Academy of Sciences ; Original Innovation Program of the Chinese Academy of Sciences ; National Key R&D Program of China ; National Key R&D Program of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Basic Research Program of Yunnan Province ; Basic Research Program of Yunnan Province ; Foundations of Yunnan Province ; Foundations of Yunnan Province ; Original Innovation Program of the Chinese Academy of Sciences ; Original Innovation Program of the Chinese Academy of Sciences ; National Key R&D Program of China ; National Key R&D Program of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Basic Research Program of Yunnan Province ; Basic Research Program of Yunnan Province ; Foundations of Yunnan Province ; Foundations of Yunnan Province ; Original Innovation Program of the Chinese Academy of Sciences ; Original Innovation Program of the Chinese Academy of Sciences |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/87688]  |
| 专题 | 中国科学院国家天文台 |
| 通讯作者 | Zhang, Pengfei |
| 作者单位 | 1.Yunnan Univ, Key Lab Astroparticle Phys Yunnan Prov, Sch Phys & Astron, Dept Astron, Kunming 650091, Yunnan, Peoples R China 2.Chinese Acad Sci, Shanghai Astron Observ, Key Lab Res Galaxies & Cosmol, 80 Nandan Rd, Shanghai 200030, Peoples R China |
| 推荐引用方式 GB/T 7714 | Zhang, Pengfei,Xing, Yi,Wang, Zhongxiang. Discovery of gamma-Ray Pulsations from PSR J1835-3259B in the Globular Cluster NGC 6652[J]. ASTROPHYSICAL JOURNAL LETTERS,2022,935(2):4. |
| APA | Zhang, Pengfei,Xing, Yi,&Wang, Zhongxiang.(2022).Discovery of gamma-Ray Pulsations from PSR J1835-3259B in the Globular Cluster NGC 6652.ASTROPHYSICAL JOURNAL LETTERS,935(2),4. |
| MLA | Zhang, Pengfei,et al."Discovery of gamma-Ray Pulsations from PSR J1835-3259B in the Globular Cluster NGC 6652".ASTROPHYSICAL JOURNAL LETTERS 935.2(2022):4. |
入库方式： OAI收割
来源：国家天文台
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