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X-Ray Astronomy
other
Editor(s):
Riccardo Giacconi
,
Herbert Gursky
Publication date
(Print):
1974
Publisher:
Springer Netherlands
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Book
ISBN (Print):
978-90-277-0387-3
ISBN (Electronic):
978-94-010-2105-0
Publication date (Print):
1974
DOI:
10.1007/978-94-010-2105-0
SO-VID:
ea69723b-141d-4e0c-949f-e28c223eae88
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Book chapters
pp. 1
Stellar and Solar Abundances
pp. 1
Introduction
pp. 3
A Linear Theory of the Perturbed Two-Body Problem (Regularization)
pp. 5
Collisional Processes in Stellar Systems
pp. 13
Polarization Clouds and Dynamical Friction
pp. 21
Collision Singularities in Gravitational Problems
pp. 25
Observational Techniques
pp. 34
Regularization Using a Time-Transformation Only
pp. 99
Mechanisms for the Production of X-Rays in a Cosmic Setting
pp. 155
X-Ray Sky
pp. 22
Relaxation Times in Strictly Disk Systems
pp. 25
Clusters in the Magellanic Clouds
pp. 38
Local Magnetic Fields on the Sun
pp. 49
Solar Motion and Velocity Distribution of a Group of Stars
pp. 169
Solar X-Ray Emission
pp. 237
Canonical Quantization of Gravity
pp. 65
The Distribution of the Residual Velocities: A Numerical Method
pp. 85
Space Distribution and State of Motion of the Early-Type Stars, Open Clusters, Associations and Stellar Rings
pp. 207
Compact X-Ray Sources
pp. 44
Monte Carlo Models of Star Clusters
pp. 267
Supernova Remnants
pp. 299
Interstellar Medium
pp. 50
Properties of the Neutral Hydrogen in the Magellanic Clouds
pp. 62
On the Lifetimes of Galactic Clusters
pp. 321
Extragalactic X-Ray Sources
pp. 359
The Cosmic X-Ray Background
pp. 85
Neutral Atmospheric Chemistry — Introduction and Review
pp. 114
Liquid Helium-Cooled Bolometers
pp. 121
A New Type of Helium-Cooled Bolometer
pp. 156
Elliptic Restricted Problem: Fourth-Order Stability Analysis of the Triangular Points
pp. 148
A Multi-Particle Regularisation Technique
pp. 319
Planetary Distances and the Missing Planet
pp. 367
Summary
pp. 373
Direct Integration Methods of the N-Body Problem
pp. 388
Treatment of Close Approaches in the Numerical Integration of the Gravitational Problem of N Bodies
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