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Near-Field Cosmology with Dwarf Elliptical Galaxies

important issues related to near-field cosmology with dwarf elliptical galaxies.;

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Dwarf Galaxies (IAU S344)

, with sections dedicated to: Local Group dwarf galaxies; the interstellar medium and star formation in dwarfs; metallicity, massive stars, and;

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The Vision of Cosmic Universe to Prem Universe-1995

Galaxies, Spherical and Elliptical Galaxies, Cosmic Functions and Cosmic Sources. How to define the Universe? Cosmic Universe beyond PREM (Field;

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Galaxy Formation and Evolution

of spiral and elliptical galaxies; central supermassive black holes and the activity associated with them; galaxy interactions; and the;

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Galaxies at High Redshift

Observational cosmology, with the help of large telescopes, combined with the capabilities of the Hubble Space Telescope and other space;

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Galaxies at High Redshift

Observational cosmology, with the help of large telescopes, combined with the capabilities of the Hubble Space Telescope and other space;

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Principles of Physical Cosmology

decades. P. J. E. Peebles provides an authoritative overview of the field, showing how observation has combined with theory to establish the;

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A Catalogue of Southern Peculiar Galaxies and Associations

ejecting material, distorted galaxies, and galaxies in near collision with each other. Volume I contains positions in right ascension and;

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Galaxy Formation

be called classical cosmology . What's more, he describes how the study of the origin of galaxies and larger-scale structures in the;

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The Properties of Star-Forming Galaxies at z~2

total masses of the galaxies. About 10% of the galaxies are apparently young starbursts with high gas fractions, caught just as they have begun;

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Cosmological Inflation and Large-Scale Structure

This textbook provides graduate students with a thorough and up-to-date introduction to inflationary cosmology. Enormous progress has been;

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Dynamics Of Galaxies

sound physical models. Next, the observational properties and models of spiral then elliptical galaxies are examined in detail. Finally, a;

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Evolution of Stars and Stellar Populations

of related techniques, that are widely applied by researchers in the field to investigate the formation and evolution of galaxies. This book will be;

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Local Group Cosmology

One of the most fascinating unresolved problems of modern astrophysics is how the galaxies we observe today were formed. The Lambda-Cold;

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Plasma Astrophysics and Cosmology

, in stars, galaxies, and clusters of galaxies, and throughout the observable universe. Plasma astrophysics and cosmology, as a unified discipline;

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We Both Read-About Space (Third Edition) (Pb) - Nonfiction

This newly revised edition provides exciting new information and spectacular photographs of planets, moons, stars and galaxies. The;

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Galaxies

, especially changes in chemical composition over time, is covered. The book concludes with a discussion of the origin of galaxies and their relation;

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AGN Feedback in Galaxy Formation

internal and external environment of their host galaxies. Featuring contributions from well-respected researchers in the field, and bringing;

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Extragalactic Astrophysics

, galaxy clustering, active galaxies, general relativity and cosmology.;

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Extragalactic Astrophysics

, galaxy clustering, active galaxies, general relativity and cosmology.;

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Adventures in Cosmology

This volume tells of the quest for cosmology as seen by some of the finest cosmologists in the world. It starts with Galaxy Formation from;

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Astrophysics of the Interstellar Medium

galaxies and galaxy clusters, the ISM is everywhere. Studying its properties is vital for the exploration of virtually any field in astronomy and;

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Astrophysics of the Interstellar Medium

galaxies and galaxy clusters, the ISM is everywhere. Studying its properties is vital for the exploration of virtually any field in astronomy and;

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Galaxies, Axisymmetric Systems and Relativity

Professor Bonnor had contributed. In particular, the influence of his work in two important fields of interest to astonomers, physicists and;

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Astronomy and Big Data

to validate the acquired results. It is concluded that a vast majority of these galaxies are, in fact, of spiral morphology with a small;

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Finite-Temperature Field Theory

cosmology cover white dwarf and neutron stars, neutrino emissivity, baryon number violation in the early universe, and cosmological phase;

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Finite-Temperature Field Theory

cosmology cover white dwarf and neutron stars, neutrino emissivity, baryon number violation in the early universe, and cosmological phase;

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