Characterizing the Gamma-Ray Emission Properties of the Globular Cluster M5 with the Fermi-LAT
文献类型：期刊论文
| 作者 | Hou, X.1,11,12; Zhang, W.9,10; Freire, P. C. C.8; Torres, D. F.7,9,10; Ballet, J.5,6; Smith, D. A.4; Johnson, T. J.2,3; Kerr, M.24; Cheung, C. C.24; Guillemot, L.22,23 |
| 刊名 | ASTROPHYSICAL JOURNAL
 |
| 出版日期 | 2024-04-01 |
| 卷号 | 964期号:2页码:118 |
| ISSN号 | 0004-637X |
| DOI | 10.3847/1538-4357/ad3210 |
| 产权排序 | 22 |
| 英文摘要 | We analyzed the globular cluster M5 (NGC 5904) using 15 yr of gamma-ray data from the Fermi Large Area Telescope (LAT). Using rotation ephemerides generated from Arecibo and FAST radio telescope observations, we searched for gamma-ray pulsations from the seven millisecond pulsars (MSPs) identified in M5. We detected no significant pulsations from any of the individual pulsars. In addition, we searched for possible variations of the gamma-ray emission as a function of orbital phase for all six MSPs in binary systems, but we did not detect any significant modulations. The gamma-ray emission from the direction of M5 is well described by an exponentially cutoff power-law spectral model, although other models cannot be excluded. The phase-averaged emission is consistent with being steady on a timescale of a few months. We estimate the number of MSPs in M5 to be between 1 and 10, using the gamma-ray conversion efficiencies for well-characterized gamma-ray MSPs in the Third Fermi-LAT Catalog of Gamma-ray Pulsars, suggesting that the sample of known MSPs in M5 is (nearly) complete, even if it is not currently possible to rule out a diffuse component of the observed gamma rays from the cluster. |
| WOS关键词 | LARGE-AREA TELESCOPE ; ALL-SKY SURVEY ; MILLISECOND PULSARS ; DYNAMICAL FORMATION ; 47 TUCANAE ; FUNDAMENTAL PLANE ; CHANDRA DETECTION ; NGC 6624 ; BINARY ; PULSATIONS |
| 资助项目 | National Aeronautics and Space Administration in the United States ; Department of Energy in the United States ; Commissariat a l'Energie Atomique in France ; Centre National de la Recherche Scientifique/Institut National de Physique Nucleaire et de Physique des Particules in France ; Agenzia Spaziale Italiana in Italy ; Istituto Nazionale di Fisica Nucleare in Italy ; Ministry of Education, Culture, Sports, Science and Technology (MEXT) in Japan ; High Energy Accelerator Research Organization (KEK) in Japan ; Japan Aerospace Exploration Agency (JAXA) in Japan ; Istituto Nazionale di Astrofisica in Italy ; K. A. Wallenberg Foundation in Sweden ; Centre National d'Etudes Spatiales in France ; Swedish Research Council in Sweden ; DOE ; Swedish National Space Board in Sweden ; [DE-AC02-76SF00515] |
| WOS研究方向 | Astronomy & Astrophysics |
| 语种 | 英语 |
| WOS记录号 | WOS:001190057600001 |
| 出版者 | IOP Publishing Ltd |
| 资助机构 | National Aeronautics and Space Administration in the United States ; Department of Energy in the United States ; Commissariat a l'Energie Atomique in France ; Centre National de la Recherche Scientifique/Institut National de Physique Nucleaire et de Physique des Particules in France ; Agenzia Spaziale Italiana in Italy ; Istituto Nazionale di Fisica Nucleare in Italy ; Ministry of Education, Culture, Sports, Science and Technology (MEXT) in Japan ; High Energy Accelerator Research Organization (KEK) in Japan ; Japan Aerospace Exploration Agency (JAXA) in Japan ; Istituto Nazionale di Astrofisica in Italy ; K. A. Wallenberg Foundation in Sweden ; Centre National d'Etudes Spatiales in France ; Swedish Research Council in Sweden ; DOE ; Swedish National Space Board in Sweden |
| 源URL | [http://ir.xao.ac.cn/handle/45760611-7/6231]  |
| 专题 | 研究单元未命名 |
| 通讯作者 | Hou, X.; Torres, D. F. |
| 作者单位 | 1.Chinese Acad Sci, Yunnan Observ, Kunming 650216, Yunnan, Peoples R China 2.Naval Res Lab, Washington, DC 20375 USA 3.George Mason Univ, Coll Sci, Fairfax, VA 22030 USA 4.Univ Bordeaux, Lab Astrophys Bordeaux, CNRS, B18N,Allee Geoffroy St Hilaire, F-33615 Pessac, France 5.CEA, CNRS, Univ Paris Cite, AIM, F-91191 Gif Sur Yette, France 6.Univ Paris Saclay, F-91191 Gif Sur Yette, France 7.ICREA, E-08010 Barcelona, Spain 8.Max Planck Inst Radioastron, Hugel 69, D-53121 Bonn, Germany 9.Inst Estudis Espacials Catalunya IEEC, Barcelona 08034, Spain 10.CSIC, Inst Space Sci ICE, Campus UAB, Barcelona 08193, Spain |
| 推荐引用方式 GB/T 7714 | Hou, X.,Zhang, W.,Freire, P. C. C.,et al. Characterizing the Gamma-Ray Emission Properties of the Globular Cluster M5 with the Fermi-LAT[J]. ASTROPHYSICAL JOURNAL,2024,964(2):118. |
| APA | Hou, X..,Zhang, W..,Freire, P. C. C..,Torres, D. F..,Ballet, J..,...&Wang, N..(2024).Characterizing the Gamma-Ray Emission Properties of the Globular Cluster M5 with the Fermi-LAT.ASTROPHYSICAL JOURNAL,964(2),118. |
| MLA | Hou, X.,et al."Characterizing the Gamma-Ray Emission Properties of the Globular Cluster M5 with the Fermi-LAT".ASTROPHYSICAL JOURNAL 964.2(2024):118. |
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