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基本説明
With a foreword by S. Chandrasekhar. Published for the first time in English translation. Contains papers relating to nebulae, papers on stellar dynamics, and more.
Full Description
This important volume contains selected papers by the celebrated astronomer Victor A. Ambartsumian, many of which are being published for the first time in English translation. The first section contains papers relating to nebulae, including his simple formulation of Zanstra's methods for determining the temperature of the central stair illuminating a planetary nebula, which led to the first treatment of the radiative equilibrium of a planetary nebula. Section 2 contains Ambartsumian's papers on Stellar dynamics, where he stresses the importance of the statistics of binary stars for the time scale of the universe, whilst Section 3 contains his work on radiative transfer, including two papers in which he formulates his principles of invariance in the theory of radiative transfer. Section 4 relates to interstellar absorption, and includes articles on the fluctuations of brightness of our Galaxy, formulated in terms of the principle of invariance, and the astronomical consequences of this principle in stellar statistics.
Contents
Stars; stellar associations; stellar association around P Cyg; preliminary data on O-associations in the galaxy; on the probability of apparent multiple systems of trapezium type; on comet-like nebulae; stellar associations and the origins of stars; stars of the T Tauri and UV Centi types and the phenomenon of continous emission; on the problem of the mechanism of the origin of stars in stellar associations; the degenerate superdense gas of elementary particles; on equilibrium configurations of superdense degenerate gas masses; the mass defect of Baryon stars; on the statistics of flare objects; percentage of flare stars among RW Aurigae type variables in the Orion association; FGuors; derivation of the frequency function of stellar flares in a star cluster; some resolutions of T Tauri stars VI galaxies; remark on the galaxy as a spiral system; some remarks on the multiple galaxies; stellar systems of positive total energy; multiple galaxies and radio galaxies III; multiple galaxies and radio galaxies IV; on the evolution of stellar systems; the George Darwin lecture for 1960-63; on the evolution of galaxies; instability phenomena in systems of galaxies; problems of extra-galactic research; superassociations in distant galaxies; some remarks on the nature of the nuclei of galaxies; on the nuclei of galaxies and their activity; opening address at the symposium "Nuclei of Galaxies"; galaxies and their nuclei miscellaneous; present status of the natural sciences and philisophy; on some trends in the development of astrophysics. Appendix - Victor Amazaspovich Ambartsumian.
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