Comparing the super-Eddington accretion of SMC X-3 and RX J0209.6-7427 with Swift J0243.6+6124
文献类型：期刊论文
| 作者 | Liu, JR ; Vasilopoulos, G; Ge, MY; Ji, L; Weng, SS; Zhang, SN; Hou, X
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| 刊名 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
 |
| 出版日期 | 2022 |
| 卷号 | 517期号:3页码:3354-3361 |
| 关键词 | accretion, accretion discs pulsars: individual: RX J0209.6 7427-pulsars: individual: SMC X-3 pulsars: individual: Swift J0243.6+6124 X-rays: binaries |
| ISSN号 | 0035-8711 |
| DOI | 10.1093/mnras/stac2746 |
| 文献子类 | Article |
| 英文摘要 | We study the giant outbursts of SMC X-3 and RX J0209.6-7427 (hereafter RX J0209) to compare their super-Eddington accretion regime with that of Swift J0243.6+6124 (hereafter Swift J0243). The high double-peak profile of SMC X-3 is found to be 0.25 phase offset from that below 2.3 x 10(38) erg s(-1), which is similar to Swift J0243 (happened around 0.9 x 10(38) erg s(-1)). The profile of RX J0209 shows a similar 0.25 phase offset between high double-peak and low double-peak around 1.25 x 10(38) erg s(-1). The 0.25 phase offset corresponds to a 90 degrees angle change of the emission beam and strongly supports for a transition from a fan beam to a pencil beam. Their critical luminosities imply a surface magnetic field similar to 4 x 10(13) and 2 x 10(13) G for SMC X-3 and RX J0209, respectively, based on the recently measured cyclotron line of Swift J0243. The spin-up rate and luminosity of SMC X-3 follows a relation of (v)over dot proportional to L-0.94(+/- 0.0)3, while that of RX J0209 follows (v)over dot proportional to L-1.00 +/-(0.03), which are similar to Swift J0243 and consistent with the prediction of a radiation-pressure-dominated disc. These results indicate that accretion columns are indeed formed above Eddington luminosity, and the population of ultraluminous X-ray pulsars likely corresponds to X-ray pulsars of highest magnetic field. |
| 电子版国际标准刊号 | 1365-2966 |
| 语种 | 英语 |
| WOS记录号 | WOS:000874073300007 |
| 源URL | [http://ir.ihep.ac.cn/handle/311005/299900]  |
| 专题 | 高能物理研究所_粒子天体物理中心 高能物理研究所_计算中心 硬X射线调制望远镜卫星 |
| 作者单位 | 中国科学院高能物理研究所 |
| 推荐引用方式 GB/T 7714 | Liu, JR,Vasilopoulos, G,Ge, MY,et al. Comparing the super-Eddington accretion of SMC X-3 and RX J0209.6-7427 with Swift J0243.6+6124[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2022,517(3):3354-3361. |
| APA | Liu, JR.,Vasilopoulos, G.,Ge, MY.,Ji, L.,Weng, SS.,...&Hou, X.(2022).Comparing the super-Eddington accretion of SMC X-3 and RX J0209.6-7427 with Swift J0243.6+6124.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,517(3),3354-3361. |
| MLA | Liu, JR,et al."Comparing the super-Eddington accretion of SMC X-3 and RX J0209.6-7427 with Swift J0243.6+6124".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 517.3(2022):3354-3361. |
入库方式： OAI收割
来源：高能物理研究所
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