High-Energy Spectroscopic Astrophysics [electronic resource] :Saas-Fee Advanced Course 30 2000. Swiss Society for Astrophysics and Astronomy / by Steven M. Kahn, Rashid A. Sunyaev, Peter Ballmoos.
by Kahn, Steven M [author.]; Sunyaev, Rashid A [author.]; Ballmoos, Peter [author.]; SpringerLink (Online service).
Material type:
Item type | Current location | Call number | Status | Date due | Barcode |
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QB460-466 (Browse shelf) | Available | ||||
QB980-991 (Browse shelf) | Available | ||||
Long Loan | MAIN LIBRARY | QB1-991 (Browse shelf) | Available |
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TP248.13-248.65 Biotechnology for Odor and Air Pollution Control | TA405-409.3 Flow and Transport in Fractured Porous Media | QB1-991 High-Energy Spectroscopic Astrophysics | QB460-466 High-Energy Spectroscopic Astrophysics | QB980-991 High-Energy Spectroscopic Astrophysics | RD1-811 Tips and Techniques in Laparoscopic Surgery | TA405-409.3 Tribo-Fatigue |
Soft X-Ray Spectroscopy of Astrophysical Plasmas (Steven M. Kahn): Classical and Quantum Radiation Theory -- The Structure of Multi-Electron Atoms -- Electron-Ion Collisional Processes -- Discrete Line Diagnostics -- Concluding Remarks -- Instruments for Nuclear Astrophysics (Peter von Ballmoos): Introduction -- Interaction of High-Energy Photons with Matter -- Detectors -- The Instruments for Nuclear Astronomy -- Hard X-Ray and Gamma Ray Spectroscopy (Rashid Sunyaev and Sergey Sazonov): Fundamentals of Compton Scattering -- Comptonization in Infinite Homogeneous Media -- Comptonization in Bounded Plasma Clouds -- Interaction of X-Rays with Partially Ionized Media -- 6.4-keV Fluorescent Emission from Molecular Clouds in the Galactic Center -- X-Ray Emission from Supernova 1987A -- Accretion onto Black Holes and Neutron Stars.
After three decades of intense research in X-ray and gamma-ray astronomy, the time was ripe to summarize basic knowledge on X-ray and gamma-ray spectroscopy for interested students and researchers ready to become involved in new high-energy missions. This volume exposes both the scientific basics and modern methods of high-energy spectroscopic astrophysics. The emphasis is on physical principles and observing methods rather than a discussion of particular classes of high-energy objects, but many examples and new results are included in the three chapters as well.
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