Galaxy Masses as Constraints of Formation Models (IAU S311)

Galaxy Masses as Constraints of Formation Models (IAU S311) PDF Author: Michele Cappellari
Publisher: Cambridge University Press
ISBN: 9781107078697
Category : Science
Languages : en
Pages : 0

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Book Description
Bringing together theorists, observers and instrumentation specialists, IAU Symposium 311 provides an overview of the techniques used to measure the masses of stars, gas and dark matter in galaxies, and explores what these mass determinations tell us about galaxy evolution. A key advance in recent years has been the enrichment of studies of the luminosity evolution of galaxies with determinations of their stellar or total masses from dynamical analyses using stellar populations, stellar or gaseous dynamical models, and weak or strong lensing. This volume addresses some of the fundamental questions in the field: what key observables can be robustly reproduced by the models? How should existing and new instrumentation be optimized for galaxy evolution studies? And, what future observations would be most useful to constrain the models? IAU S311 offers a valuable insight into this rapidly developing and interdisciplinary area of study, for researchers and graduate students.

Galaxy Masses as Constraints of Formation Models (IAU S311)

Galaxy Masses as Constraints of Formation Models (IAU S311) PDF Author: Michele Cappellari
Publisher: Cambridge University Press
ISBN: 9781107078697
Category : Science
Languages : en
Pages : 0

Get Book Here

Book Description
Bringing together theorists, observers and instrumentation specialists, IAU Symposium 311 provides an overview of the techniques used to measure the masses of stars, gas and dark matter in galaxies, and explores what these mass determinations tell us about galaxy evolution. A key advance in recent years has been the enrichment of studies of the luminosity evolution of galaxies with determinations of their stellar or total masses from dynamical analyses using stellar populations, stellar or gaseous dynamical models, and weak or strong lensing. This volume addresses some of the fundamental questions in the field: what key observables can be robustly reproduced by the models? How should existing and new instrumentation be optimized for galaxy evolution studies? And, what future observations would be most useful to constrain the models? IAU S311 offers a valuable insight into this rapidly developing and interdisciplinary area of study, for researchers and graduate students.

Nucleosynthesis and Chemical Evolution of Galaxies

Nucleosynthesis and Chemical Evolution of Galaxies PDF Author: Bernard Ephraim Julius Pagel
Publisher: Cambridge University Press
ISBN: 0521840309
Category : Science
Languages : en
Pages : 485

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Book Description
A lucid introduction for advanced undergraduates and graduate students, and an authoritative overview for researchers and professional scientists.

The Evolution of The Milky Way

The Evolution of The Milky Way PDF Author: Francesca Matteucci
Publisher: Springer Science & Business Media
ISBN: 9401009384
Category : Science
Languages : en
Pages : 605

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Book Description
This review of the most up-to-date observational and theoretical information concerning the chemical evolution of the Milky Way compares the abundances derived from field stars and clusters, giving information on the abundances and dynamics of gas.

Modern Statistical Methods for Astronomy

Modern Statistical Methods for Astronomy PDF Author: Eric D. Feigelson
Publisher: Cambridge University Press
ISBN: 052176727X
Category : Science
Languages : en
Pages : 495

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Book Description
Modern Statistical Methods for Astronomy: With R Applications.

Astronomy and Astrophysics Monthly Index

Astronomy and Astrophysics Monthly Index PDF Author:
Publisher:
ISBN:
Category : Astronomy
Languages : en
Pages : 764

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Book Description


Panchasiddhantika.

Panchasiddhantika. PDF Author: Varma Mihira
Publisher: Legare Street Press
ISBN: 9781015563735
Category : Mathematics
Languages : en
Pages : 0

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Book Description
This work has been selected by scholars as being culturally important, and is part of the knowledge base of civilization as we know it. This work is in the "public domain in the United States of America, and possibly other nations. Within the United States, you may freely copy and distribute this work, as no entity (individual or corporate) has a copyright on the body of the work. Scholars believe, and we concur, that this work is important enough to be preserved, reproduced, and made generally available to the public. We appreciate your support of the preservation process, and thank you for being an important part of keeping this knowledge alive and relevant.

An Introduction to Galaxies and Cosmology

An Introduction to Galaxies and Cosmology PDF Author: David John Adams
Publisher: Cambridge University Press
ISBN: 9780521546232
Category : Science
Languages : en
Pages : 452

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Book Description
This introductory textbook has been designed by a team of experts for elementary university courses in astronomy and astrophysics. It starts with a detailed discussion of the structure and history of our own Galaxy, the Milky Way, and goes on to give a general introduction to normal and active galaxies including models for their formation and evolution. The second part of the book provides an overview of the wide range of cosmological models and discusses the Big Bang and the expansion of the Universe. Written in an accessible style that avoids complex mathematics, and illustrated in colour throughout, this book is suitable for self-study and will appeal to amateur astronomers as well as undergraduate students. It contains numerous helpful learning features such as boxed summaries, student exercises with full solutions, and a glossary of terms. The book is also supported by a website hosting further teaching materials.

The Origin and Evolution of Galaxies

The Origin and Evolution of Galaxies PDF Author: J.T. Jones
Publisher: Springer Science & Business Media
ISBN: 9400979398
Category : Science
Languages : en
Pages : 359

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Book Description
The Origin and Evolution of Galaxies is the outstanding problem of modern cosmology. Fortunately. we have a firm cosmological framework on which to base our theories (the hot big bang) and recently there has been substantial progress in providing observations which potentially can constrain these theories. The problem of galaxy formation is. as a consequence. one involving many diverse branches of physics and astrophysics. It has been the aim of the school. and this compendium of lectures and seminars. to bring together these diverse aspects at a level enabling research workers to understand what is going on in other corners of the subject and to see how progress in each area impinges on the others. We are grateful to the contributors to this volume for allowing us considerable editorial license with their articles. We have attempted to provide a representative sample of the talks that were given at the school besides the texts of the invited lecturers. It is regrettable that for reasons of space we have had to leave out a number of other contributions.

Geometry, Topology, and Dynamics in Negative Curvature

Geometry, Topology, and Dynamics in Negative Curvature PDF Author: C. S. Aravinda
Publisher: Cambridge University Press
ISBN: 110752900X
Category : Mathematics
Languages : en
Pages : 378

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Book Description
Ten high-quality survey articles provide an overview of important recent developments in the mathematics surrounding negative curvature.

Physics and Chemistry of Comets

Physics and Chemistry of Comets PDF Author: Walter F. Huebner
Publisher: Springer Science & Business Media
ISBN: 3642748058
Category : Science
Languages : en
Pages : 389

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Book Description
As this excellent book demonstrates, the study of comets has now reached the fas cinating stage where we understand comets in general simple tenns while, at the same time, we are uncertain about practically all the details of cometary nature, structure, processes, and origin. In every aspect, even including dynamics, a choice among several or many competing theories is made impossible simply by the lack of detailed knowledge. The space missions, snapshot studies of two comets, partic ularly the one that immortalizes the name of Sir Edmund Halley, have produced a huge mass of valuable new infonnation and a number of surprises. Nonetheless, we face the tantalizing realization that we have obtained only a fleeting glance at two of perhaps a hundred billion (lOll) or more comets with possibly differing natures, origins, and physical histories. To my personal satisfaction, comets seem to have discrete nuclei made up of dirty snowballs, as I concluded four decades ago, but perhaps they are more like frozen rubbish piles.