papertrans
发表于 2025-3-21 19:28:25
书目名称Isolated Neutron Stars: From the Surface to the Interior影响因子(影响力)<br> http://impactfactor.cn/if/?ISSN=BK0475752<br><br> <br><br>书目名称Isolated Neutron Stars: From the Surface to the Interior影响因子(影响力)学科排名<br> http://impactfactor.cn/ifr/?ISSN=BK0475752<br><br> <br><br>书目名称Isolated Neutron Stars: From the Surface to the Interior网络公开度<br> http://impactfactor.cn/at/?ISSN=BK0475752<br><br> <br><br>书目名称Isolated Neutron Stars: From the Surface to the Interior网络公开度学科排名<br> http://impactfactor.cn/atr/?ISSN=BK0475752<br><br> <br><br>书目名称Isolated Neutron Stars: From the Surface to the Interior被引频次<br> http://impactfactor.cn/tc/?ISSN=BK0475752<br><br> <br><br>书目名称Isolated Neutron Stars: From the Surface to the Interior被引频次学科排名<br> http://impactfactor.cn/tcr/?ISSN=BK0475752<br><br> <br><br>书目名称Isolated Neutron Stars: From the Surface to the Interior年度引用<br> http://impactfactor.cn/ii/?ISSN=BK0475752<br><br> <br><br>书目名称Isolated Neutron Stars: From the Surface to the Interior年度引用学科排名<br> http://impactfactor.cn/iir/?ISSN=BK0475752<br><br> <br><br>书目名称Isolated Neutron Stars: From the Surface to the Interior读者反馈<br> http://impactfactor.cn/5y/?ISSN=BK0475752<br><br> <br><br>书目名称Isolated Neutron Stars: From the Surface to the Interior读者反馈学科排名<br> http://impactfactor.cn/5yr/?ISSN=BK0475752<br><br> <br><br>
令人发腻
发表于 2025-3-21 22:45:16
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认识
发表于 2025-3-22 00:41:18
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预防注射
发表于 2025-3-22 07:16:48
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Engaged
发表于 2025-3-22 11:02:10
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FIN
发表于 2025-3-22 15:03:59
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关节炎
发表于 2025-3-22 18:20:11
,The continuum and line spectra of SGR 1806-20 bursts, feature. We examined whether theses spectral lines are dependent upon the choice of a particular continuum model and find no such dependence. Besides, we find that the 5 keV feature is pronounced with high confidence in the cumulative joint spectrum of the entire burst sample, both in the individua
Diverticulitis
发表于 2025-3-22 23:11:08
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chemoprevention
发表于 2025-3-23 02:56:21
,The anatomy of a magnetar: XMM monitoring of the transient anomalous X-ray pulsar XTE J1810–197,s now consistent with the previous lack of detected pulsations in quiescence. We also summarize the detections of radio emission from XTE J1810–197, the first confirmed for any AXP. We consider possible models for the emission geometry and mechanisms of XTE J1810–197.
commonsense
发表于 2025-3-23 06:10:47
,PSR J1119–6127 and the X-ray emission from high magnetic field radio pulsars,e emission has been found in high-magnetic-field radio pulsars, the X-ray characteristics of PSR J1119–6127 require alternate models from those of conventional thermal emission from neutron stars. In addition, PSR J1119–6127 is now the radio pulsar with the smallest characteristic age from which the