標題: Titlebook: Black Holes in Binaries and Galactic Nuclei: Diagnostics, Demography and Formation; Proceedings of the E Lex Kaper,Edward P. J. van den Heu [打印本頁] 作者: deliberate 時間: 2025-3-21 19:54
書目名稱Black Holes in Binaries and Galactic Nuclei: Diagnostics, Demography and Formation影響因子(影響力)
書目名稱Black Holes in Binaries and Galactic Nuclei: Diagnostics, Demography and Formation影響因子(影響力)學科排名
書目名稱Black Holes in Binaries and Galactic Nuclei: Diagnostics, Demography and Formation網(wǎng)絡(luò)公開度
書目名稱Black Holes in Binaries and Galactic Nuclei: Diagnostics, Demography and Formation網(wǎng)絡(luò)公開度學科排名
書目名稱Black Holes in Binaries and Galactic Nuclei: Diagnostics, Demography and Formation被引頻次
書目名稱Black Holes in Binaries and Galactic Nuclei: Diagnostics, Demography and Formation被引頻次學科排名
書目名稱Black Holes in Binaries and Galactic Nuclei: Diagnostics, Demography and Formation年度引用
書目名稱Black Holes in Binaries and Galactic Nuclei: Diagnostics, Demography and Formation年度引用學科排名
書目名稱Black Holes in Binaries and Galactic Nuclei: Diagnostics, Demography and Formation讀者反饋
書目名稱Black Holes in Binaries and Galactic Nuclei: Diagnostics, Demography and Formation讀者反饋學科排名
作者: palliative-care 時間: 2025-3-22 00:17 作者: 金盤是高原 時間: 2025-3-22 02:01
,Theorien zu Unternehmensübernahmen,ll stellar motions are very close to isotropy. They indicate a central mass concentration with a density . M. pc. that dominates the potential between 0.01 and 1 pc. The derived mass ranges between 2.6 and 3.3 x 10. M. for a distance of 8.0 kpc. Such a mass concentration cannot be stable and must be作者: 催眠 時間: 2025-3-22 05:22 作者: Addictive 時間: 2025-3-22 10:42 作者: atrophy 時間: 2025-3-22 13:18 作者: agonist 時間: 2025-3-22 20:42
Hans-Gert Penzel,Christian PietigThe maximum mass of neutron stars is one of the most important predictions of the general relativistic theory of stellar structure. This paper highlights the difficulties in making a definitive prediction, and also reviews the progress made so far.作者: 搖曳的微光 時間: 2025-3-23 00:59
David Fubini,Colin Price,Maurizio ZolloThe advent of the large effective apertures of the Keck telescopes has resulted in the determination with unprecedented accuracy of the mass functions and mass ratios of faint (. mag) X-ray transients (GS 2000+25, GRO J0422+32, Nova Oph 1977, Nova Vel 1993).作者: ILEUM 時間: 2025-3-23 03:24 作者: 全部逛商店 時間: 2025-3-23 05:47 作者: Cognizance 時間: 2025-3-23 12:58
Begriffe, Formen, Regulierungen,New subarcsecond data on NGC 3227 and NGC 1068 obtained with the Plateau de Bure millimeter interferometry indicate large enclosed masses and the possibility of warped molecular gas disks.作者: Frisky 時間: 2025-3-23 17:18 作者: CHANT 時間: 2025-3-23 18:05
Keck Observations of Black Hole X-Ray Transients,The advent of the large effective apertures of the Keck telescopes has resulted in the determination with unprecedented accuracy of the mass functions and mass ratios of faint (. mag) X-ray transients (GS 2000+25, GRO J0422+32, Nova Oph 1977, Nova Vel 1993).作者: 時間等 時間: 2025-3-24 01:51
Optical Spectroscopic Observations of Black-Hole Candidates,All observations were made using the Double-Beam Spectrograph on the 2.3m telescope at Siding Spring. See Table 1 for a log of observations. Both the red and blue sides were utilised together with the D1 dichroic mirror. All spectra were reduced using the standard reduction techniques in IRAF.作者: 神經(jīng) 時間: 2025-3-24 05:13 作者: 不自然 時間: 2025-3-24 09:14
Molecular Gas in Nuclei of the Seyfert Galaxies NGC3227 and NGC1068,New subarcsecond data on NGC 3227 and NGC 1068 obtained with the Plateau de Bure millimeter interferometry indicate large enclosed masses and the possibility of warped molecular gas disks.作者: 彎曲的人 時間: 2025-3-24 10:48
Overview: Black Holes in the Universe,soon be able to measure black hole spins. We are now in a position to study the formation and demography of black holes, and to develop a deeper understanding of how they interact with their environments.作者: Allege 時間: 2025-3-24 15:56
YALO Observations of 4U 1543-47,- Ohio State) 1 meter telescope at Cerro Tololo. The folded light curves show clean amplitudes of 0.05 mag in ., 0.03 mag in ., and < 0.02 mag in .. We discuss models of the light curves and present updated and refined system parameters.作者: FIR 時間: 2025-3-24 21:06 作者: 熱心 時間: 2025-3-25 03:13
978-3-662-30799-1Springer-Verlag Berlin Heidelberg 2001作者: 消瘦 時間: 2025-3-25 04:05
Developing the Mereology of Chemistryful enterprises. I am truly touched by the honor you have wanted to do me by organizing this symposium. The only fly in the ointment for me has been that Lex Kaper had convinced me to give a talk before I realized what was happening. Between the recent physical move to the U.S. with my papers in tra作者: 課程 時間: 2025-3-25 10:18
Einleitung: Jede Industrie ist im Endgame,soon be able to measure black hole spins. We are now in a position to study the formation and demography of black holes, and to develop a deeper understanding of how they interact with their environments.作者: Coronary 時間: 2025-3-25 13:59 作者: 出來 時間: 2025-3-25 18:06 作者: aggrieve 時間: 2025-3-25 21:07 作者: 一再遛 時間: 2025-3-26 02:42 作者: AFFIX 時間: 2025-3-26 04:21 作者: Additive 時間: 2025-3-26 12:25 作者: 真實的人 時間: 2025-3-26 16:06
https://doi.org/10.1007/978-3-030-99842-4estigations using long slit spectroscopic data have yielded strong evidence for the presence of a massive dark object of ca. 10. solar masses. NGC 3115 therefore appears to be a prominent candidate for hosting a black hole in its center. . We demonstrate that with integral field spectroscopy the rot作者: trigger 時間: 2025-3-26 16:55
,Theorien zu Unternehmensübernahmen,n a search for supermassive black holes. This talk concentrates on the data reduction process and the difficulties which have to be overcome to obtain reliable kinematic measurements from STIS observations. Our analysis is based on standard STIS-pipeline software (GSFC’s IDL version of the CALSTIS p作者: 美麗的寫 時間: 2025-3-27 00:32 作者: Strength 時間: 2025-3-27 03:36 作者: 多樣 時間: 2025-3-27 05:43 作者: 即席 時間: 2025-3-27 12:00
Begriffe, Formen, Regulierungen,ifferences in their radiation and power density spectra. The efficiency of energy release due to accretion onto a rotating neutron star usually is higher than in the case of a black hole. The theory of the spreading layer on the surface of an accreting neutron star is discussed. It predicts the appe作者: pulmonary-edema 時間: 2025-3-27 17:35 作者: attenuate 時間: 2025-3-27 20:18
Einleitung: Jede Industrie ist im Endgame,soon be able to measure black hole spins. We are now in a position to study the formation and demography of black holes, and to develop a deeper understanding of how they interact with their environments.作者: Antimicrobial 時間: 2025-3-27 22:46
Teilnahmeentscheidungen im M&A-Markt,- Ohio State) 1 meter telescope at Cerro Tololo. The folded light curves show clean amplitudes of 0.05 mag in ., 0.03 mag in ., and < 0.02 mag in .. We discuss models of the light curves and present updated and refined system parameters.作者: compel 時間: 2025-3-28 04:15
ESO Astrophysics Symposiahttp://image.papertrans.cn/b/image/188947.jpg作者: 慌張 時間: 2025-3-28 08:54 作者: 爭論 時間: 2025-3-28 11:54 作者: Calculus 時間: 2025-3-28 18:19 作者: 巡回 時間: 2025-3-28 20:00
Begriffe, Formen, Regulierungen,regions of normal spiral galaxies, using the near-infrared H and K band CO stellar absorption features. Integral field data from SINFONI will provide high-resolution two-dimensional maps of nuclear velocity dispersion and rotation, which in turn will constrain the anisotropy parameter and yield robust estimates of the central dark mass.作者: sphincter 時間: 2025-3-29 02:50 作者: 繞著哥哥問 時間: 2025-3-29 06:25
Graeme K. Deans,Fritz Kr?ger,Stefan Zeiselct object masses. This is accomplished via optical and IR photometry and spectroscopy of the mass-losing star during the extended X-ray quiescent periods, exploiting essentially classical binary astronomy techniques. I will summarise the optical and IR properties of these objects and review some of the more recent results.作者: Budget 時間: 2025-3-29 08:17
,Dimensionen von Zusammenschlüssen,is above the canonical ., viz., Vela X-1, for which a mass close to . is found. Prospects for progress appear brightest for studies of systems in which the neutron star should have accreted substantial amounts of matter.作者: 察覺 時間: 2025-3-29 15:16
https://doi.org/10.1007/978-3-030-99842-45 therefore appears to be a prominent candidate for hosting a black hole in its center. . We demonstrate that with integral field spectroscopy the rotation and velocity dispersion can be much better constrained by sampling in both spatial dimensions. This yields revised and more secure results.作者: 慷慨援助 時間: 2025-3-29 19:35 作者: anticipate 時間: 2025-3-29 22:32
Black Holes in X-Ray Binaries,ct object masses. This is accomplished via optical and IR photometry and spectroscopy of the mass-losing star during the extended X-ray quiescent periods, exploiting essentially classical binary astronomy techniques. I will summarise the optical and IR properties of these objects and review some of the more recent results.作者: Hemiplegia 時間: 2025-3-30 00:11 作者: BALE 時間: 2025-3-30 04:09
Effects of Anisotropy on the Central Dark Mass in NGC 3115. New Results from Integral Field Spectro5 therefore appears to be a prominent candidate for hosting a black hole in its center. . We demonstrate that with integral field spectroscopy the rotation and velocity dispersion can be much better constrained by sampling in both spatial dimensions. This yields revised and more secure results.作者: 的事物 時間: 2025-3-30 09:19 作者: Deject 時間: 2025-3-30 13:22
Developing the Mereology of Chemistryomee viewgraphs to share with you. I was sustained in the thought (I believe due to Pascal) that one should not underestimate the pleasure that people have in listening to something they already know.作者: 相信 時間: 2025-3-30 16:55 作者: 演講 時間: 2025-3-30 23:48 作者: Sigmoidoscopy 時間: 2025-3-31 04:52
,Towards Complete Stellar Orbits Around the Galaxy’s Central Black Hole: The First Acceleration Measlack hole, but have also permitted us to begin to constrain the orbits of these stars, which appear to be bound to the central mass. Continued study of these orbits (which possibly have periods as short as 10 years) will allow us to infer the radial distribution of dark matter within a few hundredths of a parsec around the black hole.作者: ARENA 時間: 2025-3-31 05:38 作者: colostrum 時間: 2025-3-31 12:57
Measuring the Mass of the Black Hole in GS2000+25 Using IR Ellipsoidal Variations,rbit is ., and when combined with the observed mass function, corresponds to a primary mass of .. More data is needed to better define the minima, fill in the small gaps in the light curve, and explore the possibility of an eccentric orbit.作者: –吃 時間: 2025-3-31 14:10
Gas/Stars Coupling in Early-Type Galaxies: Diagnostics for Supermassive Black Holes,gas and stellar components in a small sample of early-type galaxies, demonstrating the need for both high resolution and bidimensional spatial coverage to understand the structure and dynamics of their central regions, and in particular to test the presence of SBHs.作者: 我還要背著他 時間: 2025-3-31 17:50
Centaurus A: The Supermassive Black Hole in the Nearest AGN,d spectra and new insights into the region around the black hole. We summarize what is known about Cen A, discuss the implications of recent HST optical and infrared imaging and polarimetry, and present some preliminary results from VLT/ISAAC.作者: 軟弱 時間: 2025-4-1 00:08 作者: 注意到 時間: 2025-4-1 04:36
Conference proceedings 2001e nuclei of galaxies, presented by leading expert astronomers. Special attention is given to the formation (including the recent evidence from gamma-ray bursts), physical properties, and demographics of black holes.作者: preeclampsia 時間: 2025-4-1 07:39
1431-2433 and in the nuclei of galaxies, presented by leading expert astronomers. Special attention is given to the formation (including the recent evidence from gamma-ray bursts), physical properties, and demographics of black holes.978-3-662-30799-1978-3-540-44562-3Series ISSN 1431-2433 Series E-ISSN 1611-6143
