Supernovae : the proceedings of a special IAU session on supernovae held on September 1, 1976 in Grenoble, France
Author(s)
Bibliographic Information
Supernovae : the proceedings of a special IAU session on supernovae held on September 1, 1976 in Grenoble, France
（Astrophysics and space science library, v. 66）
D. Reidel, c1977
Available at 19 libraries
Note
"Held in conjunction with the International Astronomical Union meeting in Grenoble, France."
Includes bibliographies
Description and Table of Contents
Description
Supernovae are among the most exciting things occurring in the universe. Much recent research has concentrated on phenomena related to supernovae. For example, the origin of the cosmic rays and the origin of the bulk of the heavy elements seem to be closely associated with the phenomenon of supernovae. With the discovery of the pulsar in the Crab, it seemed clear that supernovae were also intimately as sociated with the formation of neutron stars and perhaps even black holes. The purpose of the conference, of which this volume contains the proceedings, was to bring together the leaders of supernova re search, each of whom has concentrated on different aspects of the problem, to try to form a coherent picture both observationally and theoretically of our current understanding of supernovae. In so doing, key invited talks were presented on the light curves of super novae, both observationally and theoretically; on the possible uses of supernovae, for example in determination of the Hubble Constant; on the formation and evolution of supernova remnants, again both ob servationally and theoretically. The possibility that supernovae might explain quasars was also presented. A review of the current status of statistics of supernovae was presented, giving the rate at which they go off and the implications with regard to what mass stars are the progenitors for supernovae. Again, this was presented both from the observational point of view and from the theoretical stellar evolution point of view.
Table of Contents
II. Observations of Supernovae at the Astrophysical Observatory of Asiago.- III. The Early Type I Supernova Light Curve: The Effect of Hydrogen Abundance.- IV. Supernovae and the Value of the Hubble Constant.- V. X-Rays from Supernova Remnants.- VI. Was SN 1054 a Type II Supernova?.- VII. The Evolution of Supernova Remnants.- VIII. Evidence for a Class of Supernova Remnants Resembling the Crab Nebula.- IX. Ionization Structure of the Cygnus Loop.- X. Supernovae and Quasars.- XI. A Progress Report on Supernova Statistics.- XII. Masses of Supernova Progenitors.- XIII. Evolution of Supernova Progenitors (SNP).- XIV. CMa R1: A Case Of Supernova-Induced Star Formation?.- XV. Supernova Nucleosynthesis.- XVI. Gravitational Collapse, Weak Interactions, and Supernova Outbursts.- XVII. Mechanisms for Supernova Explosions.
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