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Chinese Academy of Sciences Institutional Repositories Grid
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CAS IR Grid
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金属研究所 [6]
国家空间科学中心 [6]
高能物理研究所 [5]
新疆天文台 [5]
紫金山天文台 [5]
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期刊论文 [36]
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2023 [1]
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The Influences of Micro-Alloying Element Sn and Magnetic Field on the Microstructure Evolution of Al-Bi Immiscible Alloys
期刊论文
OAI收割
METALS, 2023, 卷号: 13, 期号: 11, 页码: 13
作者:
Chen, Shu
;
Jiang, Hongxiang
;
Zhao, Jiuzhou
  |  
收藏
  |  
浏览/下载:24/0
  |  
提交时间:2024/01/07
alloying element
magnetic field
solidification
microstructure evolution
Timing and evolution of PSR B0950+08
期刊论文
OAI收割
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2022, 卷号: 512, 期号: 4, 页码: 4689-4696
作者:
Huang, Hai-tao
;
Zhou, Xia
;
Yuan, Jian-ping
;
Zheng, Xiao-Ping
  |  
收藏
  |  
浏览/下载:30/0
  |  
提交时间:2022/07/28
stars: evolution
stars: magnetic field
stars: neutron
pulsars: individual: PSR B0950+08
The magnetized white dwarf plus helium star binary evolution with accretion-induced collapse
期刊论文
OAI收割
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2021, 卷号: 509, 期号: 4, 页码: 6061-6067
作者:
Ablimit, Iminhaji
  |  
收藏
  |  
浏览/下载:48/0
  |  
提交时间:2022/09/19
binaries: close
stars: evolution
stars: magnetars
stars: magnetic field
pulsars: general
supernovae: general
white dwarfs
High plasma cut-off frequency blocks the radio emission from accreting millisecond X-ray pulsar SAX J1808.4-3658
期刊论文
OAI收割
Astrophysics and Space Science, 2020, 卷号: 365, 期号: 3, 页码: 47
作者:
Wang, S. Q.
;
Zhang, C. M.
;
Wang, D. H.
;
Wang, N.
;
Wang, J. B.
  |  
收藏
  |  
浏览/下载:26/0
  |  
提交时间:2021/04/12
(Stars:) pulsar: individual: SAX J1808.4-3658
Stars
neutron
X-rays
stars
X-rays
binaries
X-rays: general
neutron-star
magnetic-field
optical counterpart
xmm-newton
binary
evolution
constraints
transient
sax-j1808.4-3658
oscillations
Astronomy & Astrophysics
The braking index of PSR B0540-69 and the associated pulsar wind nebula emission after spin-down rate transition
期刊论文
OAI收割
Monthly Notices of the Royal Astronomical Society, 2020, 卷号: 494, 页码: 1865-1870
作者:
HXMT
  |  
收藏
  |  
浏览/下载:57/0
  |  
提交时间:2022/02/08
stars: magnetic field
stars: neutron
pulsars: general
Astrophysics
- High Energy Astrophysical Phenomena
Abstract: In 2011 December, PSR B054-69 experienced a spin-down rate transition (SRT), after which the spin-down power of the pulsar increased by $\sim 36{{\ \rm per\ cent}}$. About 1000 d after the SRT, the X-ray luminosity of the associated pulsar wind nebula (PWN) was found to brighten by $32\pm 8{{\ \rm per\ cent}}$. After the SRT, the braking index n of PSR B0540-69 changes from n = 2.12 to 0.03 and then keeps this value for about five years before rising to n = 0.9 in the following years. We find that most of the current models have difficulties in explaining the measured braking index. One exceptive model of the braking index evolution is the increasing dipole magnetic field of PSR B0540-69. We suggest that the field increase may result from some instabilities within the pulsar core that enhance the poloidal component at the price of toroidal component of the magnetic field. The increasing dipole magnetic field will result in the X-ray brightening of the PWN. We fit the PWN X-ray light curve by two models: one assumes a constant magnetic field within the PWN during the brightening and the other assumes an enhanced magnetic field proportional to the energy density of the PWN. It appears that the two models fit the data well, though the later model seems to fit the data a bit better. This provides marginal observational evidence that magnetic field in the PWN is generated by the termination shock. Future high-quality and high-cadence data are required to draw a solid conclusion.
Unifying neutron star sub-populations in the supernova fallback accretion model
期刊论文
iSwitch采集
Research in astronomy and astrophysics, 2019, 卷号: 19, 期号: 3, 页码: 12
作者:
Liu, Bai-Sheng
;
Li, Xiang-Dong
收藏
  |  
浏览/下载:196/0
  |  
提交时间:2019/04/22
Accretion, accretion disks
Stars: neutron, evolution, rotation, magnetic field, magnetars
Pulsars: general
Unifying neutron star sub-populations in the supernova fallback accretion model
期刊论文
iSwitch采集
Research in astronomy and astrophysics, 2019, 卷号: 19, 期号: 3, 页码: 12
作者:
Liu, Bai-Sheng
;
Li, Xiang-Dong
收藏
  |  
浏览/下载:196/0
  |  
提交时间:2019/04/22
Accretion, accretion disks
Stars: neutron, evolution, rotation, magnetic field, magnetars
Pulsars: general
Solidification of Immiscible Alloys Under the Effect of Electric and Magnetic Fields
期刊论文
OAI收割
ACTA METALLURGICA SINICA-ENGLISH LETTERS, 2018, 卷号: 31, 期号: 12, 页码: 1240-1248
作者:
Jiang, HX
;
Zhao, JZ
  |  
收藏
  |  
浏览/下载:220/0
  |  
提交时间:2018/12/25
Immiscible alloys
Solidification
Microstructure evolution
Electric current
Magnetic field
Electric-magnetic fields
Solidification of Immiscible Alloys Under the Effect of Electric and Magnetic Fields
期刊论文
OAI收割
ACTA METALLURGICA SINICA-ENGLISH LETTERS, 2018, 卷号: 31, 期号: 12, 页码: 1240-1248
作者:
Jiang, Hong-Xiang
;
Zhao, Jiu-Zhou
  |  
收藏
  |  
浏览/下载:21/0
  |  
提交时间:2021/02/02
Immiscible alloys
Solidification
Microstructure evolution
Electric current
Magnetic field
Electric-magnetic fields