×
验证码:
换一张
忘记密码?
记住我
CORC
首页
科研机构
检索
知识图谱
申请加入
托管服务
登录
注册
在结果中检索
科研机构
高能物理研究所 [100]
内容类型
期刊论文 [98]
影音 [2]
发表日期
2021 [2]
2020 [2]
2019 [6]
2018 [17]
2017 [19]
2016 [4]
更多...
学科主题
Astronomy... [39]
Astronomy ... [1]
Physics [1]
×
知识图谱
CORC
开始提交
已提交作品
待认领作品
已认领作品
未提交全文
收藏管理
QQ客服
官方微博
反馈留言
浏览/检索结果:
共100条,第1-10条
帮助
限定条件
专题:高能物理研究所
第一署名单位
第一作者单位
通讯作者单位
已选(
0
)
清除
条数/页:
5
10
15
20
25
30
35
40
45
50
55
60
65
70
75
80
85
90
95
100
排序方式:
请选择
作者升序
作者降序
题名升序
题名降序
发表日期升序
发表日期降序
提交时间升序
提交时间降序
Luminosity Dependence of the Cyclotron Line Energy in 1A 0535+262 Observed by Insight-HXMT during the 2020 Giant Outburst
期刊论文
The Astrophysical Journal, 2021, 卷号: 917, 页码: L38
作者:
Kong, L. D.
;
Zhang, S.
;
Ji, L.
;
Reig, P.
;
Doroshenko, V.
收藏
  |  
浏览/下载:10/0
  |  
提交时间:2021/11/18
X-ray astronomy
High mass x-ray binary stars
Pulsars
1810
733
1306
Astrophysics - High Energy Astrophysical Phenomena
Physical origin of the non-physical spin evolution of MAXI J1820 + 070
期刊论文
Monthly Notices of the Royal Astronomical Society, 2021, 卷号: 504, 页码: 2168
作者:
Guan, J.
;
Tao, L.
;
Qu, J. L.
;
Zhang, S. N.
;
Zhang, W.
收藏
  |  
浏览/下载:61/0
  |  
提交时间:2021/11/18
accretion
accretion discs
black hole physics
stars: individual
(MAXI J1820 + 070)
X-rays: binaries
Astrophysics - High Energy
Astrophysical Phenomena
83C57
The braking index of PSR B0540-69 and the associated pulsar wind nebula emission after spin-down rate transition
期刊论文
Monthly Notices of the Royal Astronomical Society, 2020, 卷号: 494, 页码: 1865-1870
作者:
HXMT
收藏
  |  
浏览/下载:15/0
  |  
提交时间:2022/02/08
stars: magnetic field
stars: neutron
pulsars: general
Astrophysics
- High Energy Astrophysical Phenomena
Insight-HXMT observations of Swift J0243.6+6124: the evolution of RMS pulse fractions at super-Eddington luminosity
期刊论文
Monthly Notices of the Royal Astronomical Society, 2020, 卷号: 497, 页码: 5498-5506
作者:
HXMT
收藏
  |  
浏览/下载:15/0
  |  
提交时间:2022/02/08
stars: neutron
pulsars: individual: Swift J0243.6+6124
X-rays:
binaries
Long-term evolutions of the cyclotron line energies in her x-1, vela x-1, and cen x-3 as observed with swift/bat
期刊论文
Monthly notices of the royal astronomical society, 2019, 卷号: 484, 期号: 3, 页码: 3797-3805
作者:
Ji, L.
;
Staubert, R.
;
Ducci, L.
;
Santangelo, A.
;
Zhang, S.
收藏
  |  
浏览/下载:64/0
  |  
提交时间:2019/04/22
Radiation mechanisms: thermal
Scattering
Stars: magnetic field
Stars: neutron
X-rays: binaries
X-rays: individual: her x-1, vela x-1, cen x-3
Long-term evolutions of the cyclotron line energies in her x-1, vela x-1, and cen x-3 as observed with swift/bat
期刊论文
Monthly notices of the royal astronomical society, 2019, 卷号: 484, 期号: 3, 页码: 3797-3805
作者:
Ji, L.
;
Staubert, R.
;
Ducci, L.
;
Santangelo, A.
;
Zhang, S.
收藏
  |  
浏览/下载:64/0
  |  
提交时间:2019/04/22
Radiation mechanisms: thermal
Scattering
Stars: magnetic field
Stars: neutron
X-rays: binaries
X-rays: individual: her x-1, vela x-1, cen x-3
Unifying neutron star sub-populations in the supernova fallback accretion model
期刊论文
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:179/0
  |  
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
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:179/0
  |  
提交时间:2019/04/22
Accretion, accretion disks
Stars: neutron, evolution, rotation, magnetic field, magnetars
Pulsars: general
Insight-HXMT Observations of Swift J0243.6+6124 during Its 20172018 Outburst
期刊论文
The Astrophysical Journal, 2019, 卷号: 879
作者:
Zhang, Wei
;
Zhang, WanChang
;
Zhang, WenZhao
;
Zhang, Yi
;
Zhang, YiFei
收藏
  |  
浏览/下载:191/0
  |  
提交时间:2019/07/12
accretion
accretion disks
pulsars: individual: Swift J0243.6+6124
stars: distances
stars: magnetic field
X-rays: binaries
Astrophysics
- High Energy Astrophysical Phenomena
Constant cyclotron line energy in Hercules X-1 - Joint Insight-HXMT and NuSTAR observations
期刊论文
Journal of High Energy Astrophysics, 2019, 卷号: 23, 页码: 29-32
作者:
HXMT
收藏
  |  
浏览/下载:33/0
  |  
提交时间:2022/02/08
Stars: neutron star
Pulsars: binary(Her X-1)
X-rays: stars
Astrophysics - High Energy Astrophysical Phenomena
Abstract: The long-term evolution of the centroid energy of the CRSF in Her X-1 is still a mystery. We report a new measurement from a campaign between Insight-HXMT and NuSTAR performed in February 2018. Generally, the two satellites show well consistent results of timing and spectral properties. The joint spectral analysis confirms that the previously observed long decay phase has ended, and that the line energy instead keeps constant around 37.5 keV after flux correction.
©版权所有 ©2017 CSpace - Powered by
CSpace