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Near-Field Cosmology with Dwarf Elliptical Galaxies (IAU C198)

Near-Field Cosmology with Dwarf Elliptical Galaxies (IAU C198)
Author: International Astronomical Union. Colloquium
Publisher: Cambridge University Press
Total Pages: 456
Release: 2005
Genre: Science
ISBN: 9780521852043

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Proceedings of IAUC 198, covering important issues related to near-field cosmology with dwarf elliptical galaxies.


Nearly Normal Galaxies

Nearly Normal Galaxies
Author: Sandra M. Faber
Publisher: Springer Science & Business Media
Total Pages: 475
Release: 2012-12-06
Genre: Science
ISBN: 1461247624

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It is sometimes said that astronomy is the crossroads of physics. In the same spirit, it can forcefully be argued that galaxies are the crossroads of astronomy. Internal pro ces ses within galaxies involve all of the fundamental components of astrophysics: stellar evolution, star formation, low-density astrophysics, dynamics, hydrodynamics, and high-energy astrophysics. Indeed, one can hardly name an observational datum in any wavelength range on any kind of celestial object that does not provide a useful clue to galaxy formation and evolution. Although internal processes in galaxies until recently occupied most of our attention, we now know that it is also vital to relate galaxies to their environment. How galaxies congregate in larger structures and are in turn influenced by them are crucial questions for galactic evolution. On a grander level we have also come to regard galaxies as the basic building blocks of the universe, the basic units whereby the large scale structure of the universe is apprehended and quantified. On a grander level still, we also believe strongly that galaxies are the direct descendents of early density irregularities in the Big Bang. Galaxy properties are now viewed as providing a crucial constraint on the physics of the Big Bang and a vital link between the macroscopic and microscopic structure of the universe.


Star Formation in Galaxies

Star Formation in Galaxies
Author:
Publisher:
Total Pages: 810
Release: 1987
Genre: Astrophysics
ISBN:

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Galaxies: Interactions and Induced Star Formation

Galaxies: Interactions and Induced Star Formation
Author: Robert C. Kennicutt Jr.
Publisher: Springer Science & Business Media
Total Pages: 417
Release: 2006-04-18
Genre: Science
ISBN: 3540316302

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This volume contains the written versions of the lectures given at the 26th course of the renowned Saas-Fee series. The book represents a comprehensive and up-to-date review of the field of galaxy interaction. Nowadays, galaxies are no longer seen as immutable objects: they evolve, interact, merge, blaze, and reshape. Dynamic forces can induce powerful stellar activity able to transform the matter composition and morphology of galaxies. The lectures included in this book aim at a better understanding of these remarkable and fascinating phenomena. Though the book is intended for graduate students and young post-docs in astrophysics, it contains more advanced and original material, as well as historical perspectives, which will be of great interest to experts and astronomy teachers also.


Physics of Star Formation in Galaxies

Physics of Star Formation in Galaxies
Author: F. Palla
Publisher: Springer Science & Business Media
Total Pages: 242
Release: 2006-07-06
Genre: Science
ISBN: 3540316337

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The book begins with a historical introduction, "Star Formation: The Early History", that presents new material of interest for students and historians of science. This is followed by two long articles on "Pre-Main-Sequence Evolution of Stars and Young Clusters" and "Observations of Young Stellar Objects". These articles on the fascinating problem of star formation from interstellar matter give a thorough overview of present-day theories and observations. The articles contain material so far unpublished in the astronomical literature. The book addresses graduate students and can be used as a textbook for advanced courses in stellar astrophysics.


The First Galaxies

The First Galaxies
Author: Tommy Wiklind
Publisher: Springer Science & Business Media
Total Pages: 434
Release: 2012-12-15
Genre: Science
ISBN: 3642323626

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New observations of the period between the cosmic recombination and the end of reionization are posing intriguing questions about where the first generations of stars were formed, how the first galaxies were assembled, whether these galaxies have low redshift counterparts, and what role the early galaxies played in the reionization process. Combining the new observational data with theoretical models can shed new light on open issues regarding the star formation process, its role in the reionization of the Universe, and the metal enrichment in galaxies at those early epochs. This volume brings together leading experts in the field to discuss our current level of understanding and what may come in the near future as our observational as well as theoretical tools improve. The book confronts the theory of how the first stars, black holes, and galaxies formed with current and planned observations. This synthesis is very timely, just ahead of the establishment of major new facilities, such as the James Webb Space Telescope (JWST), a next-generation, millimeter/sub-millimeter observatory in the Atacama desert (ALMA), and ground-based Extremely Large Telescopes (ELT). Together, they will revolutionize the study of the most distant objects in the Universe. This volume is aimed at beginning graduate students but can also serve as a reference work for active researchers in the field. Apart from presenting the fundamental concepts involved, it also provides an introduction to the methods and techniques used. The book will also be useful to anyone with an astrophysical background who needs an effective starting point for learning about the first stars and galaxies.


Physical Processes in Fragmentation and Star Formation

Physical Processes in Fragmentation and Star Formation
Author: Roberto Capuzzo-Dolcetta
Publisher: Springer Science & Business Media
Total Pages: 462
Release: 2012-12-06
Genre: Science
ISBN: 9400906056

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Recent years have witnessed the expansion and multiplication of the observations of star formation and fragmentation accompanied by a consequent growth in the study of the underlying physical processes, the chemistry, the sites, the times, etc. Moreover, recent studies have shown that the formation of stars is likely to share many features with the formation of other self-gravitating objects. The present volume, therefore, discusses the formation of such objects in a systematic and comparative manner.