A clear and accessible introduction to quantum mechanical methods used to calculate properties of atoms exposed to strong magnetic fields in both laboratory and stellar environments, with the emphasis on hydrogen and helium and their isoelectronic sequences. The results of the detailed calculations are listed in tables, making it a useful handbook for astrophysicists and atomic physicists alike.
This volume is published in honor of Friedrich Hund's 100th birthday. It is a modern review on matter at high densities and pressures in astrophysics from Hund's early contribution to present-day ideas. The relation between the equation of state and the structure of compact cosmic objects is discussed, and two main contributions deal with the equation of state of baryonic matter at nuclear densities and with the numerical solution of the general relativistic field equations for non-rotating and rapidly rotating neutron stars. In a final chapter the present state of asteroseismology is presented as a tool to explore the interior of cosmic objects by analyzing the observed free oscillations of the Earth, the Sun, and white dwarf stars.
This volume is published in honor of Friedrich Hund's 100th birthday. It is a modern review on matter at high densities and pressures in astrophysics from Hund's early contribution to present-day ideas. The relation between the equation of state and the structure of compact cosmic objects is discussed, and two main contributions deal with the equation of state of baryonic matter at nuclear densities and with the numerical solution of the general relativistic field equations for non-rotating and rapidly rotating neutron stars. In a final chapter the present state of asteroseismology is presented as a tool to explore the interior of cosmic objects by analyzing the observed free oscillations of the Earth, the Sun, and white dwarf stars.
A clear and accessible introduction to quantum mechanical methods used to calculate properties of atoms exposed to strong magnetic fields in both laboratory and stellar environments, with the emphasis on hydrogen and helium and their isoelectronic sequences. The results of the detailed calculations are listed in tables, making it a useful handbook for astrophysicists and atomic physicists alike.
This volume presents in compact form main persons and press organs in the history of the American media system, described by Pulitzer Prize Winners. There are personality profiles of press tycoons like Joseph Pulitzer, William Randolph Hearst and Henry Luce as key figures. There are other press founders like Alexander Hamilton, creator of the `New York Evening Post', or Henry Raymond who established the `New York Times'. There also are sketches about originally bankrupt newspapers sold at auctions and became successful under new publishers, like the `New York World' or the `Washington Post'. Other chapters cover high-circulation publications as exemplified by the `Ladies' Home Journal' or `Time' magazine. In addition, several early stages of news distribution in the United States are told as well as basic press philosophies by starjournalists like Walter Lippmann. Heinz-Dietrich Fischer, EdD, PhD, is Professor Emeritus at the Ruhr-University of Bochum, Germany.
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