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Black Hole Research Past and Future | 3 | |
Overview: Black Holes in the Universe | 16 | |
Black Holes in X-Ray Binaries | 27 | |
Neutron Star Mass Determinations | 39 | |
On the Limiting Mass of Neutron Stars | 45 | |
Keck Observations of Black Hole X-Ray Transients | 53 | |
Measuring the Mass of the Black Hole in GS2000+25 Using IR Ellipsoidal Variations | 57 | |
YALO Observations of 4U 1543-47 | 59 | |
Optical Spectroscopic Observations of Black-Hole Candidates | 61 | |
The Center of the Galaxy: Evidence for a Massive Black Hole | 63 | |
Towards Complete Stellar Orbits Around the Galaxy's Central Black Hole: The First Acceleration Measurements | 72 | |
Evidence for Massive Black Holes in Nearby Galactic Nuclei | 78 | |
Effects of Anisotropy on the Central Dark Mass in NGC 3315. New Results from Integral Field Spectroscopy | 88 | |
Black-Hole Results from STIS | 91 | |
Gas/Stars Coupling in Early-Type Galaxies: Diagnostics for Supermassive Black Holes | 95 | |
Molecular Gas in Nuclei of the Seyfert Galaxies NGC3227 and NGC1068 | 99 | |
Centaurus A: The Supermassive Black Hole in the Nearest AGN | 101 | |
SINFONI - Galaxy Dynamics at 0".05 Resolution with the VLT | 107 | |
Accretion onto Black Holes and Neutron Stars: Differences and Similarities | 113 | |
X-Ray Variability of Neutron Stars versus Black Holes | 125 | |
RXTE Monitoring of LMC X-3 | 131 | |
Monitoring the Short-Term Variability of Cyg X-1 | 133 | |
Simultaneous Infrared and mm-Wave Observations of Disc Ejection Events in GRS 1915+105 | 135 | |
Observations of Cygnus X-3 in Quiescence in the 2.4 - 12 [mu]m Range with ISO | 137 | |
Determination of Mass Limits Around Pulsars at 10 and 90 [mu]m with ISO | 139 | |
X-Ray Spectra of Neutron Stars vs. Black Holes | 141 | |
Why Do Black-Hole X-Ray Binaries Tend to Be Transient? | 149 | |
Black-Hole Transients and the Eddington Limit | 155 | |
Limits on Accretion Rates in Black Hole X-Ray Transients | 159 | |
Supermassive Black Holes Can Hardly Be "Silent" | 161 | |
Discovery of an X-Ray Outburst in an Optically Non-Active Galaxy | 168 | |
The Giant X-Ray Flare of NGC5905 - a Tidal Disruption Event? | 170 | |
A Giant, Ultra-Soft, and Luminous X-Ray Flare from the Optically Inactive Galaxy Pair RX J1242.6-1119 | 172 | |
New Evidence for Supermassive Binary Black Holes in the Blazar OJ287 | 174 | |
Gravitational Lens Diagnosis of Quasar Accretion Disk | 176 | |
X-Ray Evidence of an AGN in the Starburst Galaxy M82 | 178 | |
Gamma-Ray Observations of Black Holes: The Prospects of INTEGRAL | 180 | |
Jets from Black-Hole Binaries and Galactic Nuclei | 185 | |
Black-Hole States and Radio-Jet Formation | 193 | |
Black Hole X-Ray Binaries: A New View on Soft-Hard Spectral Transitions | 200 | |
Orbital, Precessional and Flaring Variability in Cygnus X-1 | 202 | |
Modelling Synchrotron Outbursts in 3C 273 | 204 | |
On the Formation of Jets | 206 | |
The Importance of Rapid Black Hole Spin in Relativistic Jet Formation | 216 | |
Radio Cores in Low-Luminosity AGN: ADAFs or Jets? | 218 | |
The Magnetic Field Configuration of Accretion Disks around Black Holes | 222 | |
The Influence of Resonant Absorption on the Fe Emission Line Profiles of Accreting Black Holes | 224 | |
X-Ray Iron Line Variability for the Model of an Orbiting Flare Above a Black Hole Accretion Disc | 226 | |
Causal Model for Relativistic Accretion Flow | 228 | |
Black Holes or Supermassive Compact Objects Without Event Horizon? | 230 | |
Outflowing Coronae Above Accretion Discs in AGN and GBH | 232 | |
Formation of Broad Line Clouds from Turbulent Shocks in the Accretion Flows of Active Galactic Nuclei | 234 | |
Wolf-Rayet Stars and Black Holes, an Overview | 239 | |
Structure of the Globular Cluster M15 and Constraints on a Massive Central Black Hole | 246 | |
Merger Rates of Black-Hole Binaries: Prospects for Gravitational-Wave Detectors | 252 | |
Central Black Holes and Galaxy Evolution | 259 | |
X-Ray Candidates for a Population of Nuclear Cores in Local Group Galaxies | 265 | |
Global X-Ray Emission and Central Properties of Early Type Galaxies | 267 | |
A New Monte Carlo Code for Dynamical Simulations of Galactic Nuclei Hosting Massive Black Holes | 269 | |
Luminosity and Mass Functions of Active Galactic Nuclei | 273 | |
Accreting Black Holes: Modelling Individual Objects and Whole Populations | 275 | |
Formation and Evolution of Black-Hole Binaries | 279 | |
Empirical Lower Mass Limit for Black-Hole Formation in a Massive Binary | 289 | |
Constraints on the Initial Mass Limit for Black-Hole Formation from the Massive X-Ray Binary Wray 977 | 295 | |
Formation of Black-Hole X-Ray Binaries with Low-Mass Donors | 299 | |
The History of Cygnus X-2 | 305 | |
Evidence of a Supernova Origin for the Black Hole in GRO J1655-40 (Nova Scorpii 1994) | 307 | |
Constraints on Mass Ejection in Black Hole Formation Derived from Black Hole X-Ray Binaries | 312 | |
A Search for the Presence of Bow Shocks around High-Mass X-Ray Binaries | 314 | |
Gamma-Ray Bursts in Relation to Black-Hole Formation | 316 | |
Black Hole Formation, Gamma-Ray Bursts, and Stellar Winds | 328 | |
Fallback in Supernovae and Black Hole Formation | 332 | |
Black-Hole Formation and Gamma-Ray Bursts | 334 | |
The Final Fate of Coalescing Binary Neutron Stars: Collapse to a Black Hole? | 344 | |
Supermassive Black Holes: Their Formation, and Their Prospects as Probes of Relativistic Gravity | 351 | |
The Formation and Evolution of Supermassive Black Holes and their Host Galaxies | 364 | |
Black Hole Formation in Dark Matter Halos | 375 | |
Author Index | 377 |
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Add Black Holes in Binaries and Galactic Nuclei: Diagnostics, Demography and Formation, The observational evidence for the existence of black holes has grown significantly over recent decades. Stellar-mass black holes are detected as X-ray sources in binary systems, while supermassive black holes, with masses more than a million times the ma, Black Holes in Binaries and Galactic Nuclei: Diagnostics, Demography and Formation to the inventory that you are selling on WonderClubX
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Add Black Holes in Binaries and Galactic Nuclei: Diagnostics, Demography and Formation, The observational evidence for the existence of black holes has grown significantly over recent decades. Stellar-mass black holes are detected as X-ray sources in binary systems, while supermassive black holes, with masses more than a million times the ma, Black Holes in Binaries and Galactic Nuclei: Diagnostics, Demography and Formation to your collection on WonderClub |