难理解
发表于 2025-3-30 10:33:16
The Camera Object and Flash Video,eak AGN found in the LINER M81 and higher luminosity Seyfert galaxies. This supports the notion of a continuous sequence of X-ray properties from the Galactic Centre through LINER galaxies to Seyferts, Likely determined by the amount of material available for accretion in the central regions.
烤架
发表于 2025-3-30 13:26:32
The future of flash in the mobile worldxies. Particular attention will be given to the remarkable similarity found between the timing properties of Seyferts and black hole X-ray binaries, including the power spectrum and the cross spectrum (time delays and coherence), and their implications for the physical processes at work in Seyferts.
我说不重要
发表于 2025-3-30 19:40:07
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反感
发表于 2025-3-30 20:47:12
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dominant
发表于 2025-3-31 02:45:44
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鸵鸟
发表于 2025-3-31 07:15:06
On the relationship between the jets from X-ray binaries and AGN,ack holes of different masses and accretion rates. The regression coefficients of this relation contain information about the nature of the X-ray emission mechanism driving the correlation. We argue that X-ray synchrotron emission from the base of the jets is unlikely to be the dominant contribution to the X-ray spectrum in most of the sources.
CRAB
发表于 2025-3-31 12:54:21
A transition in the accretion properties of AGN,diative inefficient accretion flows. The (so far) qualitative analogy with the behavior of XRB provides an interesting perspective to find a unique framework for the accretion and jet production in accreting black hole systems.
Minuet
发表于 2025-3-31 15:59:55
A fundamental plane of black hole activity: Pushing forward the unification scheme,s between the radio (..) and the X-ray (..) luminosity and the black hole mass (.). We find that the radio luminosity is correlated with . and .., at a highly significant level. We show how this result can be used to extend the standard unification by orientation scheme to encompass unification by mass and accretion rate.
陶醉
发表于 2025-3-31 20:21:46
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土坯
发表于 2025-3-31 22:10:13
Rapid X-ray variability of Seyfert 1 Galaxies,xies. Particular attention will be given to the remarkable similarity found between the timing properties of Seyferts and black hole X-ray binaries, including the power spectrum and the cross spectrum (time delays and coherence), and their implications for the physical processes at work in Seyferts.