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Hot Stars in the Galactic Halo

evolution and the stellar populations of other galaxies. The study of hot stars in the halo of our Galaxy is undergoing an exciting renaissance;

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Co-ordination Of Galactic Research

Originally published in 1955, this book contains the noted discussions of a conference on the co-ordination of galactic research, which;

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Galaxies

is followed by two chapters on observations of galaxies, including our own. There are then three chapters on galactic structure: the manner in which;

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Gamma-ray and Neutrino Signatures of Galactic Cosmic-ray Accelerators

This book addresses three "hot" topics concerning the general problem of the origin of Galactic cosmic rays, namely (1) the acceleration;

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Galactic Dynamics in the Era of Large Surveys (IAU S353)

Galactic dynamics is fundamental to understanding the formation of galaxies, their internal evolution and their current structure. While;

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Primordial Nuclei and Their Galactic Evolution

This volume gives an overview of knowledge about the light nuclei created in the Hot Early Universe: H, D, 3He, 4He, and 7Li. It combines;

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Dynamics and Evolution of Galactic Nuclei

: supermassive black holes. Connected to the evolution of the galaxies that contain these black holes, galactic nuclei are the sites of uniquely;

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Dynamics and Evolution of Galactic Nuclei

: supermassive black holes. Connected to the evolution of the galaxies that contain these black holes, galactic nuclei are the sites of uniquely;

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Topics in Cosmic-Ray Astrophysics

physics before accelerators were built. Still later, it became astrophysics -- studying the Galactic sources of the lower energy cosmic rays, the;

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From Luminous Hot Stars to Starburst Galaxies

Luminous hot stars represent the extreme upper mass end of normal stellar evolution. Before exploding as supernovae, they live out their;

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General Assembly Of Galaxy Halos IAU S31

reviews on state-of-the-art research, covering fields such as first stars, galactic archaeology, stellar halos in cosmological simulations;

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Secular Evolution Of Galaxies

. It plays an important role in the evolution of spiral galaxies with major consequences for galactic bulges, the transfer of angular momentum;

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Cambridge Astrophysics

Luminous hot stars represent the extreme upper mass end of normal stellar evolution. Before exploding as supernovae, they live out their;

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First Book of Stars

, because the sky is too bright. The Sun is a star, and seems so bright and hot only because it is much closer than the other stars. If it were just;

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Search for neutrinos from stellar gravitational collapse with the MACRO experiment at Gran Sasso

subject of this thesis is the search for neutrino bursts from galactic stellar gravitational collapses performed in the MACRO experiment, a large;

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Understanding the Epoch of Cosmic Reionization

of Reionization. The light from these galactic ancestors began spreading out, ionizing virtually every atom in existence. Our Universe transitioned from;

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Elements and the Cosmos

In recent years there have been substantial advances in abundance analysis of stars, planetary nebulae and the interstellar medium due to;

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The Early Type Stars

and of galactic structure. Perhaps one of the simplest reasons for writing a book about the early type stars is to see if some of the;

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Einde inhoud

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