Next:
Introduction
Previous:
Cover
The Scenario Machine: Binary Star Population Synthesis
Introduction
Observational Zoo of Binaries with Compact Stars
Evolutionary Scenarios of Binary Systems
Principal Evolutionary States of Normal Stars
Main-sequence stars (stage I)
Post main sequence stars (stage II)
Roche lobe overflow (stage III)
Wolf-Rayet and He stars (stage IV)
Stellar Winds From Normal Stars
Change of Binary Parameters: Mass, Semi-major Axis and
Eccentricity
Mass change
Semi-major axis change
Special Cases: Supernova Explosion and the Common Envelope
``Ecology'' of Magnetic Rotators
A Gravimagnetic Rotator
The Environment of the Rotator
The Stopping Radius
The Stopping Radius in the Supercritical Case
Effect of the Magnetic Field
The Corotation Radius
Nomenclature
A Universal Diagram for Gravimagnetic Rotators
The Gravimagnetic Parameter
Evolution of Magnetic Rotators
The evolution equation
The equilibrium period
Evolutionary Tracks
Evolution of Magnetic Rotators in Non-circular Orbits
Mixing types of E-P-A binary systems with non-zero orbital
eccentricity
Ejector-propeller hysteresis
E-P transitions for different orbits
The Scenario Machine: Operational Guide
Notes on Monte-Carlo Simulations
Dependence on the Scenario Parameters and Initial Distributions
How to Catch ``Rare'' Tracks
Principles of Scenario Machine Operation
Calculation of Evolutionary Tracks
Initial Distributions of Binary Parameters
Star Formation Rate and Normalization of Stellar Populations
Restrictions on the Scenario Parameters
Basic Observational Data for Determination of
f(q)
and
The COOC Criterion (Criterion of Observations versus
Calculations)
Test of the Initial Mass-Ratio Distribution
Phenomenological Kick Velocity
The Effect of Kick Velocity on Binary Pulsar Populations
Binary Pulsar Diversity and High Neutron Star Birth Velocity
X-ray Galactic Sources and Binary Radiopulsars as Probes of the Initial Mass Ratio
f(q)
and Kick Velocity
w
Artificial Galaxy: Full Matrix of Stages
Massive X-ray Binaries
Ejectors in Massive Binary Systems
The Evolutionary Status of Radiopulsars in Massive Binary
Systems
The Number of Ejectors in Binaries
Why do Radiopulsars not Usually Form Pairs with Normal Stars?
Caverns in Binary Systems
The Effect of Relativistic Wind on Accretion Flow Parameters
The Radiopulsar PSRB1259-63 - a Probe in the Stellar Wind Plasma
Why must a radiopulsar coupled with an optical star have high
eccentricity?
The ``Reflection'' Effect
Other Candidates for Ejecting Stars in Binary Systems
Cyg X-3
Periodic radiosource LSI+61 303
Black Holes in Binaries
Black Hole Creation in Massive Binary Systems
Binary Radiopulsars with Black Holes
Cyg X-1 as a Progenitor of BH+PSR Binaries
PSR B0042-73 in the Small Magellanic Cloud
X-ray Luminosity Evolution
Cosmic Rays and Evolution of Binary
Systems
Supernova Explosions
Radiopulsars as Sources of Cosmic Rays
Population Synthesis of X-ray Sources at the Galactic Center
The Model
Results
Discussion and Conclusions
Sky in Gravitational Waves
Gravitational Wave Sky: An Overview
Model of the Galaxy
Frequency distribution of galactic binaries
Structure of the Galaxy
Transparency of the Stochastic Background
Galactic Gravitational Wave Background
Extragalactic Gravitational Wave Background
Gravitational Wave Background from Individual Galaxies
Critical Frequencies and Gravitational Wave Detector Halfwidth for Extragalactic Observations
Amplitude Distribution
A Gravitational Wave Map of Nearby Galaxies
Gravitational waves from supernova explosions
Gravitational Waves from Coalescing Compact Binary Stars
Gravitational wave background from nearby galaxies
Evolution of Supernova Explosion Rates in the Universe
The Supernovae Rates
-
Dependence for the Supernova Explosions
-
for Supernova Explosions
Results and Discussion
Evolution of the Double Neutron Star
Merging Rate andthe Cosmological Origin of Gamma-ray Burst Sources
Calculation of Binary Neutron Star Coalescence Rates
Effect of sources evolution on
-
distribution and
-test
Conclusions
Concluding Remarks and Future Prospects
References
Index
About this document ...
Mike E. Prokhorov
Sat Feb 22 18:38:13 MSK 1997