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Titlebook: Highlights of Astronomy; As Presented at the Jacqueline Bergeron (General Secretary of the Unio Book 1992 Springer Science+Business Media

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楼主: Monomania
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Peter L. Smithfamily, whose remarkable accomplishments in a politically hostile but scientifically rewarding environment deserve greater recognition..Haas was a fellow student of both Lise Meitner and Erwin Schrödinger and was also one of the last doctoral students of Ludwig Boltzmann. Following Boltzmann‘s suici
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P. Gillinghamand key protagonists during the early twentieth century.Desc.The book highlights the personal and scientific struggles of Arthur Erich Haas (1884-1941), an Austrian Physicist from a wealthy Jewish middle-class family, whose remarkable accomplishments in a politically hostile but scientifically rewar
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Gravitational Lensingniverse and affects our physical understanding of various classes of extragalactic objects. We summarize here part of the theoretical and observational evidences supporting these claims..After briefly reviewing the history of gravitational lenses, we recall the basic principles underlying the format
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Voyager: A Retrospectiveong with their satellites and their rings. The science return from these two spacecraft forever changed our views of this remote region of our solar system. Often overlooked, however, is the incremental gain in knowledge from these encounters over that which had been known in the early 1970s when th
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Diffuse Interstellar Clouds measurements. The focus of this review is on spectroscopic work involving atomic and molecular lines. From these measurements, the physical and chemical makeup of the clouds is derived. Here we stress that technological advances have influenced our perception of diffuse clouds.
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Cosmic Backgrounda probe of cosmology. Stringent limits can be set on the amplitude of fluctuations of the potential energy at the surface of last scattering of the CMB photons. Large angular scale (>1°) fluctuations in the gravitational potential energy are directly related to temperature anisotropies in the CMB by
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