標(biāo)題: Titlebook: From X-ray Binaries to Quasars: Black Holes on All Mass Scales; T. J. Maccarone,R. P. Fender,L. C. Ho Book 2005 Springer Science+Business [打印本頁] 作者: Adentitious 時(shí)間: 2025-3-21 16:36
書目名稱From X-ray Binaries to Quasars: Black Holes on All Mass Scales影響因子(影響力)
書目名稱From X-ray Binaries to Quasars: Black Holes on All Mass Scales影響因子(影響力)學(xué)科排名
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書目名稱From X-ray Binaries to Quasars: Black Holes on All Mass Scales網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱From X-ray Binaries to Quasars: Black Holes on All Mass Scales被引頻次
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書目名稱From X-ray Binaries to Quasars: Black Holes on All Mass Scales讀者反饋
書目名稱From X-ray Binaries to Quasars: Black Holes on All Mass Scales讀者反饋學(xué)科排名
作者: 疏忽 時(shí)間: 2025-3-21 21:37 作者: FATAL 時(shí)間: 2025-3-22 00:31
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作者: Ergots 時(shí)間: 2025-3-22 06:59 作者: Awning 時(shí)間: 2025-3-22 11:53
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作者: 字形刻痕 時(shí)間: 2025-3-22 14:42 作者: Feature 時(shí)間: 2025-3-22 17:18 作者: Liberate 時(shí)間: 2025-3-22 21:23
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作者: Exposition 時(shí)間: 2025-3-23 01:52
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作者: OGLE 時(shí)間: 2025-3-23 06:36
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作者: 展覽 時(shí)間: 2025-3-23 12:24
Broad iron lines in AGN and X-ray binaries,led analysis of these objects shows that the emission line is not significantly affected by absorption and that the source variability is principally due to variation in amplitude of a power-law. Underlying this is a much less variable, relativistically-smeared, reflection-dominated, component which作者: 微塵 時(shí)間: 2025-3-23 15:42 作者: 一個(gè)攪動(dòng)不安 時(shí)間: 2025-3-23 19:01
Rapid X-ray variability of Seyfert 1 Galaxies,e powered by a supermassive black hole fed from an accretion disc. However, since . there has been little opportunity to advance our understanding of the most rapid X-ray variability. Observations with . have changed this..We discuss some recent results obtained from . observations of Seyfert 1 gala作者: Ceremony 時(shí)間: 2025-3-23 22:55
Epicyclic frequencies derived from the effective potential: Simple and practical formulae, spacetimes. Such spacetimes include as special cases analytically known black hole Kerr and Schwarzschild spacetimes, as well as the analytic Hartle-Thorne spacetime and all numerically constructed spacetimes relevant for rotating neutron stars. Our derivation follows directly from energy and angul作者: 去才蔑視 時(shí)間: 2025-3-24 05:44
X-ray periodicity in AGN,ed from long EUVE light curves of moderate-luminosity Seyfert galaxies; the fourth was discovered in Chandra data from the low-luminosity Seyfert 1 galaxy NGC 4395. When compared with Cyg X-1, I find that the period is related to the luminosity as . ∝ .. rather than the expected one-to-one relations作者: 巨大沒有 時(shí)間: 2025-3-24 08:11 作者: buoyant 時(shí)間: 2025-3-24 11:47 作者: Concerto 時(shí)間: 2025-3-24 17:59
X-ray and radio monitoring of GX 339-4 and CYG X-1,y agrees with the IR flux level. Corbel and Fender [2002, . 573, L35—L39] later showed that the typical hard state radio power-law extrapolated forward in energy meets the backward extrapolated X-ray power-law at an IR spectral break, which was explicitly observed twice in GX 339-4. This has been ci作者: Scleroderma 時(shí)間: 2025-3-24 20:56 作者: Baffle 時(shí)間: 2025-3-25 01:55
Springer Science+Business Media B.V. 2005作者: characteristic 時(shí)間: 2025-3-25 06:52 作者: 急急忙忙 時(shí)間: 2025-3-25 11:24
The Camera Object and Flash Video,r, it will be stressed that this behavior does seem to be present in an analogous way both in radio-loud and radio-quiet AGN, as inferred from samples selected in an independent way. The found bimodality can be naturally — although not uniquely — interpreted in the frame of the ADIOS solution for ra作者: 易于 時(shí)間: 2025-3-25 12:16 作者: Adjourn 時(shí)間: 2025-3-25 17:36 作者: 多節(jié) 時(shí)間: 2025-3-25 23:49 作者: Herpetologist 時(shí)間: 2025-3-26 01:32
Alternative FLV Creation Tools, which the strong, well-ordered fields play a more important role than weak, turbulent fields. In the low/hard state this flow is interior to the standard ADAF usually invoked to explain the observed hot, optically thin emission. Preliminary solutions for these new MDAFs are presented..Time-dependen作者: 過分自信 時(shí)間: 2025-3-26 08:03
https://doi.org/10.1007/978-1-4302-0151-9ems share many common physical characteristics. The observed outflows in the micro-quasar GRS 1915+105, the Seyfert 1 galaxy MCG-6-30-15 and the Seyfert 2 galaxy IRAS 18325-5926 are the focus of this proceeding.作者: 職業(yè)拳擊手 時(shí)間: 2025-3-26 09:55
Choosing and Playing Multiple Videos,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作者: 熟練 時(shí)間: 2025-3-26 16:23
The Camera Object and Flash Video,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作者: 性上癮 時(shí)間: 2025-3-26 20:24
Choosing and Playing Multiple Videos,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作者: 慢慢啃 時(shí)間: 2025-3-26 22:10
Alternative FLV Creation Tools,led analysis of these objects shows that the emission line is not significantly affected by absorption and that the source variability is principally due to variation in amplitude of a power-law. Underlying this is a much less variable, relativistically-smeared, reflection-dominated, component which作者: 原始 時(shí)間: 2025-3-27 03:57
The future of flash in the mobile worldxte). We focus on the global evolution and the observed state transitions. Rather than giving a numerical recipe for classifying observations, we try to identify times during outbursts at which clear changes occur in the X-ray variability, X-ray spectral, or multi-wavelength properties.作者: 翅膀拍動(dòng) 時(shí)間: 2025-3-27 08:23 作者: allergen 時(shí)間: 2025-3-27 10:21
The future of flash in the mobile world spacetimes. Such spacetimes include as special cases analytically known black hole Kerr and Schwarzschild spacetimes, as well as the analytic Hartle-Thorne spacetime and all numerically constructed spacetimes relevant for rotating neutron stars. Our derivation follows directly from energy and angul作者: ANTE 時(shí)間: 2025-3-27 14:39 作者: 罵人有污點(diǎn) 時(shí)間: 2025-3-27 21:39
Flash lite mobile entertainment basicsion disk in a nonlinear 3:2 resonance. An . = 0 vertical oscillation near a black hole modulates the X-ray emission through gravitational lensing (light-bending) at the source. Certain oscillations of the accretion disk will also modulate the mass accretion rate, and in neutron-star systems this wou作者: angiography 時(shí)間: 2025-3-28 00:07
Flash lite mobile entertainment basicsk holes. In particular at frequencies <100 Hz, their power spectra can be strikingly similar. The highest frequency phenomena (kilohertz QPOs, black hole high-frequency QPOs and neutron star hectohertz QPOs) are the ones that showmost differences, perhaps because they originate closest to the compac作者: 宏偉 時(shí)間: 2025-3-28 05:09 作者: 恭維 時(shí)間: 2025-3-28 09:45 作者: chronology 時(shí)間: 2025-3-28 10:54 作者: 官僚統(tǒng)治 時(shí)間: 2025-3-28 17:18
https://doi.org/10.1007/978-1-4302-0151-9We have recently put forward a ‘unified’ semi-empirical model for the coupling between accretion and jet production in galactic black hole X-ray binaries. In this paper, we summarise this model and briefly discuss relevant considerations that have arisen since its publication.作者: Sputum 時(shí)間: 2025-3-28 20:18
A unified model for black hole X-ray binary jets?,We have recently put forward a ‘unified’ semi-empirical model for the coupling between accretion and jet production in galactic black hole X-ray binaries. In this paper, we summarise this model and briefly discuss relevant considerations that have arisen since its publication.作者: aspersion 時(shí)間: 2025-3-28 23:12
T. J. Maccarone,R. P. Fender,L. C. HoContains articles by world-leading experts.Provides articles not found anywhere else.Includes many review-type articles that are useful for students trying to get a broad view of accretion-powered obj作者: 四指套 時(shí)間: 2025-3-29 06:40 作者: Merited 時(shí)間: 2025-3-29 10:38 作者: 確定 時(shí)間: 2025-3-29 12:48
The future of flash in the mobile worldxte). We focus on the global evolution and the observed state transitions. Rather than giving a numerical recipe for classifying observations, we try to identify times during outbursts at which clear changes occur in the X-ray variability, X-ray spectral, or multi-wavelength properties.作者: Inferior 時(shí)間: 2025-3-29 17:30 作者: 終點(diǎn) 時(shí)間: 2025-3-29 22:00
https://doi.org/10.1007/978-1-4302-0151-9ack 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.作者: Anemia 時(shí)間: 2025-3-30 03:53
The Camera Object and Flash Video,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.作者: 懶洋洋 時(shí)間: 2025-3-30 04:26 作者: 難理解 時(shí)間: 2025-3-30 10:33
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.作者: 烤架 時(shí)間: 2025-3-30 13:26
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.作者: 我說不重要 時(shí)間: 2025-3-30 19:40 作者: 反感 時(shí)間: 2025-3-30 20:47 作者: dominant 時(shí)間: 2025-3-31 02:45 作者: 鴕鳥 時(shí)間: 2025-3-31 07:15
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.作者: CRAB 時(shí)間: 2025-3-31 12:54
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.作者: Minuet 時(shí)間: 2025-3-31 15:59
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.作者: 陶醉 時(shí)間: 2025-3-31 20:21 作者: 土坯 時(shí)間: 2025-3-31 22:10
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.作者: 用手捏 時(shí)間: 2025-4-1 05:43 作者: caldron 時(shí)間: 2025-4-1 08:30
X-ray periodicity in AGN,hip. This result might be explained if the QPO is associated with the inner edge of the optically thick accretion disk, and the inner-edge radius depends on the source luminosity (or black hole mass).Adiscussion of uncertainties in the period detection methodology is also discussed.作者: 聽覺 時(shí)間: 2025-4-1 12:42 作者: 說笑 時(shí)間: 2025-4-1 16:13
Book 2005 new movement to make use of the relative advantages of studying stellar mass and supermassive black holes and to bring together the knowledge gained from the two approaches. The topics discussed here run the gamut of the state of the art in black hole observational and theoretical work-variability,作者: Inscrutable 時(shí)間: 2025-4-1 18:33 作者: 凝視 時(shí)間: 2025-4-2 01:17 作者: 紳士 時(shí)間: 2025-4-2 06:17 作者: humectant 時(shí)間: 2025-4-2 09:39
Flash lite mobile entertainment basics are caused by the same physics in all three source types, this does indicate that basic properties of the accretion flow which are the same in all three source types play an important role in generating at least some of the frequencies.
