The optical/ultraviolet excess of isolated neutron stars in the resonant cyclotron scattering model
文献类型：期刊论文
| ; | |
| 作者 | Tong H(仝号); Ren-Xin Xu; Song LM(宋黎明)
|
| 刊名 | Research in Astronomy and Astrophysics;2011;第12期;P1371-1376;
 ; Research in Astronomy and Astrophysics;2011;第12期;P1371-1376;
|
| 关键词 | Hao China Tong School of Physics and State Key Laboratory of Nuclear Physics and Technology Ren-Xin Xu Li-Ming Song（Institute of High Energy Physics Chinese Academy of Sciences Beijing 100049 Peking University Beijing 100871 China） Hao China Tong School of Physics and State Key Laboratory of Nuclear Physics and Technology Ren-Xin Xu Li-Ming Song（Institute of High Energy Physics Chinese Academy of Sciences Beijing 100049 Peking University Beijing 100871 China） |
| 通讯作者 | 仝号 ; 仝号 |
| 英文摘要 | X-ray dim isolated neutron stars are peculiar pulsar-like objects,characterized by their Planck-like spectrum.In studying their spectral energy distributions,optical/ultraviolet(UV) excess is a long standing problem.Recently Kaplan et al.measured the optical/UV excess for all seven sources,which is understandable in the resonant cyclotron scattering(RCS) model previously addressed.The RCS model calculations show that the RCS process can account for the observed optical/UV excess for most sources.The ?at spectrum of RX J2143.0+0654 may be due to contributions from the bremsstrahlung emission of the electron system in addition to the RCS process.; X-ray dim isolated neutron stars are peculiar pulsar-like objects,characterized by their Planck-like spectrum.In studying their spectral energy distributions,optical/ultraviolet(UV) excess is a long standing problem.Recently Kaplan et al.measured the optical/UV excess for all seven sources,which is understandable in the resonant cyclotron scattering(RCS) model previously addressed.The RCS model calculations show that the RCS process can account for the observed optical/UV excess for most sources.The ?at spectrum of RX J2143.0+0654 may be due to contributions from the bremsstrahlung emission of the electron system in addition to the RCS process. |
| 公开日期 | 2016-02-25 |
| 源URL | [http://ir.ihep.ac.cn/handle/311005/218075]  |
| 专题 | 高能物理研究所_粒子天体物理中心 |
| 推荐引用方式 GB/T 7714 | Tong H,Ren-Xin Xu,Song LM. The optical/ultraviolet excess of isolated neutron stars in the resonant cyclotron scattering model, The optical/ultraviolet excess of isolated neutron stars in the resonant cyclotron scattering model[J]. Research in Astronomy and Astrophysics;2011;第12期;P1371-1376;, Research in Astronomy and Astrophysics;2011;第12期;P1371-1376;. |
| APA | 仝号,Ren-Xin Xu,&宋黎明. |
| MLA | 仝号,et al."The optical/ultraviolet excess of isolated neutron stars in the resonant cyclotron scattering model".Research in Astronomy and Astrophysics;2011;第12期;P1371-1376; |
入库方式： OAI收割
来源：高能物理研究所
浏览0
下载0
收藏0
其他版本
除非特别说明，本系统中所有内容都受版权保护，并保留所有权利。