Adentitious
发表于 2025-3-21 16:36:31
书目名称From X-ray Binaries to Quasars: Black Holes on All Mass Scales影响因子(影响力)<br> http://figure.impactfactor.cn/if/?ISSN=BK0163697<br><br> <br><br>书目名称From X-ray Binaries to Quasars: Black Holes on All Mass Scales影响因子(影响力)学科排名<br> http://figure.impactfactor.cn/ifr/?ISSN=BK0163697<br><br> <br><br>书目名称From X-ray Binaries to Quasars: Black Holes on All Mass Scales网络公开度<br> http://figure.impactfactor.cn/at/?ISSN=BK0163697<br><br> <br><br>书目名称From X-ray Binaries to Quasars: Black Holes on All Mass Scales网络公开度学科排名<br> http://figure.impactfactor.cn/atr/?ISSN=BK0163697<br><br> <br><br>书目名称From X-ray Binaries to Quasars: Black Holes on All Mass Scales被引频次<br> http://figure.impactfactor.cn/tc/?ISSN=BK0163697<br><br> <br><br>书目名称From X-ray Binaries to Quasars: Black Holes on All Mass Scales被引频次学科排名<br> http://figure.impactfactor.cn/tcr/?ISSN=BK0163697<br><br> <br><br>书目名称From X-ray Binaries to Quasars: Black Holes on All Mass Scales年度引用<br> http://figure.impactfactor.cn/ii/?ISSN=BK0163697<br><br> <br><br>书目名称From X-ray Binaries to Quasars: Black Holes on All Mass Scales年度引用学科排名<br> http://figure.impactfactor.cn/iir/?ISSN=BK0163697<br><br> <br><br>书目名称From X-ray Binaries to Quasars: Black Holes on All Mass Scales读者反馈<br> http://figure.impactfactor.cn/5y/?ISSN=BK0163697<br><br> <br><br>书目名称From X-ray Binaries to Quasars: Black Holes on All Mass Scales读者反馈学科排名<br> http://figure.impactfactor.cn/5yr/?ISSN=BK0163697<br><br> <br><br>
疏忽
发表于 2025-3-21 21:37:30
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FATAL
发表于 2025-3-22 00:31:23
Jet-disc coupling in the accreting black hole XTE J1118+480,ting synchrotron radiation in the optical band.We propose a scenario in which the jet and the X-ray corona are fed by the same energy reservoir where large amounts of accretion power are stored before being channelled into either the jet or the high energy radiation. This time-dependent model reprod
Ergots
发表于 2025-3-22 06:59:53
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Awning
发表于 2025-3-22 11:53:31
A fundamental plane of black hole activity: Pushing forward the unification scheme,X-ray and radio bands. We compile a sample of ∼100 active galactic nuclei with measured mass, 5 GHz core emission, and 2–10 keV luminosity, together with eight galactic black holes with a total of ∼50 simultaneous observations in the radio and X-ray bands. Using this sample, we study the correlation
字形刻痕
发表于 2025-3-22 14:42:52
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Feature
发表于 2025-3-22 17:18:05
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Liberate
发表于 2025-3-22 21:23:56
Black hole spin in AGN and GBHCs,ess with which X-ray spectroscopy can be used to probe strong gravity, we summarize how these techniques can constrain black hole spin. In particular, we highlight . studies of the Seyfert galaxy MCG-6-30-15 and the stellarmass black hole GX 339-4. The broad X-ray iron line profile, together with re
Exposition
发表于 2025-3-23 01:52:27
The Seyfert-liner galaxy NGC 7213: An , observation,on lines from Fe I, Fe . and Fe . and a soft X-ray collisionally ionised thermal plasma with . = 0.18. keV. We find a luminosity of 7 × 10. L., and a lack of soft X-ray excess emission, suggesting a truncated accretion disc. NGC 7213 has intermediate X-ray spectral properties, between those of the w
OGLE
发表于 2025-3-23 06:36:17
Observational effects of strong gravity,nt horizon. As such, these photons are subject to general relativistic effects such as light-bending, gravitational lensing and redshift, time-dilation, etc. These gravitational effects are well-understood from a theoretical standpoint and therefore, provide a natural mechanism to test the propertie