Supernovae

For millennia mankind has watched as the heavens move in their stately progression from night to night and from year to year, presaging with their changes the changing seasons. The sun, the moon, and the planets move in what appears to be an unchanging firmament, except occasionally when a new "...

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Bibliographic Details
Other Authors: Petschek, Albert G. (Editor)
Format: eBook
Language:English
Published: New York, NY Springer New York 1990, 1990
Edition:1st ed. 1990
Series:Astronomy and Astrophysics Library
Subjects:
Online Access:
Collection: Springer Book Archives -2004 - Collection details see MPG.ReNa
Table of Contents:
  • 8.3. Some General Considerations
  • 8.4. Carbon Deflagration
  • 8.5. Carbon Detonation
  • 8.6. Type Ib Supernovae
  • 8.7. Type I21 Supernovae
  • 8.8. Conclusions
  • References
  • 9 Supernovae: The Direct Mechanism and the Equation of State
  • 9.1. Introduction
  • 9.2. Gravitational Collapse
  • 9.3. Subsaturation Density Equation of State
  • 9.4. Suprasaturation Density Equation of State
  • 9.5. Numerical Results
  • 9.6. Rotation
  • 9.7. Discussion
  • References
  • 10 Neutrino Heating Supernovae
  • 10.1. Introduction
  • 10.2. Brief Review of Numerical Work
  • 10.3. Collapse-Driven Supernova
  • 10.4. Calculational Neutrino Spectra and Luminosity from Collapsed Stellar Cores
  • 10.5. The Neutrino Heating Mechanism for Supernova Explosions: A Critique
  • References
  • 1 Classification of Supernovae
  • 1.1. Introduction
  • 1.2. Observed Time Dependence
  • 1.3. Theory
  • 1.4. SN 1987K
  • 1.5. Conclusions
  • References
  • 2 Spectra of Supernovae
  • 2.1. Introduction
  • 2.2. Historical Overview
  • 2.3. Individual Supernovae: Spectral Types and Bibliography
  • 2.4. Spectrum Formation
  • 2.5. Spectral Types Ia, Ib, and II
  • 2.6. Toward Quantitative Spectroscopy
  • References
  • 3 Supernova Light Curves
  • 3.1. Introduction
  • 3.2. Light Curves of Type IA Supernovae
  • 3.3. The Light Curves of SN Ib
  • 3.4. The Cosmological Uses of SN Ia
  • 3.5. Light Curves for SN II
  • 3.6. Cosmology and SN II
  • References
  • 4 Radio Supernovae
  • 4.1. Introduction
  • 4.2. Radio Emission from SN 1970G
  • 4.3. Further Radio Detections of Type II Supernovae
  • 4.4. Radio Detection of Type I Supernovae
  • 4.5. Supernovae Discovered by Their Radio Emission
  • 4.6. Intermediate Age Radio Supernovae
  • 4.7. Very Early Radio Emission from SN 1987A
  • 4.8. Summary of Radio Supernovae
  • 4.9. Models for the Supernova Radio Emission
  • 4.10. Conclusion
  • References
  • 5 Interaction of Supernovae with Circumstellar Matter
  • 5.1. Introduction
  • 5.2. Circumstellar Environments
  • 5.3. Hydrodynamic Interaction
  • 5.4. Radiative Interaction
  • 5.5. Summary and Future Prospects
  • References
  • 6 Gamma-Rays and X-Rays from Supernovae
  • 6.1. Introduction
  • 6.2. Prompt Emission, Radiation from Interaction with a Wind, and Very High-Energy Radiation
  • 6.3. Gamma-Rays and X-Rays due to Radioactive Decay
  • 6.4. SN 1987A
  • 6.5. Concluding Remarks
  • References
  • 7 Neutrinos from Supernovae
  • 7.1. Introduction
  • 7.2. A Short History of Supernova Neutrino Theory
  • 7.3. The Neutrino Signature of Core Collapse Supernovae
  • 7.4. The Neutrinos from SN 1987A
  • Appendix: Detectors
  • References
  • 8 Type I Supernovae: Carbon Deflagration and Detonation
  • 8.1. Introduction
  • 8.2. The Pre-Explosive Evolution