chemical evolution of galaxies

作者：Francesca Matteucci 出版社：Springer Verlag 出版日：2012/01/04 裝訂：精裝

The term “chemical evolution of galaxies” refers to the evolution of abundances of chemical species in galaxies, which is due to nuclear processes occurring in stars and to gas flows into and out of g

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2.

Nucleosynthesis and Chemical Evolution of Galaxies

作者：Bernard E. J. Pagel 出版社：Cambridge Univ Pr 出版日：2009/02/02 裝訂：精裝

The distribution of elements in the cosmos is the result of many processes, and it provides a powerful tool to study the Big Bang, the density of baryonic matter, nucleosynthesis and the formation and evolution of stars and galaxies. Covering many exciting topics in astrophysics and cosmology, this textbook, by a pioneer of the field, provides a lucid and wide-ranging introduction to the interdisciplinary subject of galactic chemical evolution for advanced undergraduates and graduate students. It is also an authoritative overview for researchers and professional scientists. This new edition includes results from recent space missions and new material on abundances from stellar populations, nebular analysis, and meteoric isotopic anomalies, and abundance analysis of X-ray gas. Simple derivations for key results are provided, together with problems and helpful solution hints, enabling the student to develop an understanding of results from numerical models and real observations.

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The Origin and Evolution of Planetary Nebulae

90折

3.

The Origin and Evolution of Planetary Nebulae

作者：Sun Kwok 出版社：Cambridge Univ Pr 出版日：2007/08/13 裝訂：平裝

This authoritative volume provides a comprehensive review of the origin and evolution of planetary nebulae. It covers all the stages of their evolution, carefully synthesizes observations from across the spectrum, and clearly explains all the key physical processes at work. Particular emphasis is placed on observations from space, using the Hubble Space Telescope, the Infrared Space Observatory, and the ROSAT satellite. This book presents a thoroughly modern understanding of planetary nebulae, integrating developments in stellar physics with the dynamics of nebular evolution. It also describes exciting possibilities such as the use of planetary nebulae in determining the cosmic distance scale, the distribution of dark matter and the chemical evolution of galaxies. This book provides graduate students with an accessible introduction to planetary nebulae, and researchers with an authoritative reference. It can also be used as an advanced text on the physics of the interstellar medium.

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定價：3119 元，優惠價：9 2807

4.

Origin and Evolution of the Elements：VOLUME4

作者：Andrew McWilliam 出版社：Cambridge Univ Pr 出版日：2004/09/23 裝訂：精裝

This comprehensive volume reviews our understanding of the origin and evolution of elements, from stellar nucleosynthesis to the chemical evolution of the cosmos. With chapters by leading authorities in the field, it describes models of how the elements are produced by stars, the nuclear processes involved, and how the quantity of elements evolved in our Galaxy and distant galaxies. The observed chemical composition of stars in different locations within our Galaxy and nearby galaxies is discussed, as are the compositions of hot and cold gases, of dust grains found between stars and in meteorites, and of the integrated light from distant galaxies and quasars. This authoritative volume is a valuable resource for graduate students and professional research astronomers.

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Origin and Evolution of the Elements(Volume 4, Carnegie Observatories Astrophysics Series)

90折

5.

Origin and Evolution of the Elements(Volume 4, Carnegie Observatories Astrophysics Series)

作者：Andrew McWilliam 出版社：Cambridge Univ Pr 出版日：2010/06/24 裝訂：平裝

This comprehensive volume reviews our understanding of the origin and evolution of elements, from stellar nucleosynthesis to the chemical evolution of the cosmos. With chapters by leading authorities in the field, it describes models of how the elements are produced by stars, the nuclear processes involved, and how the quantity of elements evolved in our Galaxy and distant galaxies. The observed chemical composition of stars in different locations within our Galaxy and nearby galaxies is discussed, as are the compositions of hot and cold gases, of dust grains found between stars and in meteorites, and of the integrated light from distant galaxies and quasars. This authoritative volume is a valuable resource for graduate students and professional research astronomers.

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定價：2664 元，優惠價：9 2398

6.

The Intriguing Life of Massive Galaxies (Iau S295)

作者：Daniel Thomas 出版社：Cambridge Univ Pr 出版日：2013/10/28 裝訂：精裝

The lives of massive galaxies are affected by many key processes, including gas accretion and star formation, feedback and quenching, black hole growth, mass assembly, galaxy mergers and interactions, chemical enrichment and stellar populations, dark matter, galaxy haloes, and satellite accretion. These proceedings of IAU Symposium 295 discuss recent progress in galaxy formation and evolution, and plan ahead for future challenges. They cover, from both theoretical and observational perspectives, the lives of massive galaxies from the formation of the first galaxies in the early Universe, through their evolution with cosmic time to massive galaxies in the local Universe. Key contributions deal with recent and near-future advances in telescope technology and massive galaxy surveys as well as computer power for large-scale simulations. IAU S295 benefits advanced students and active researchers who need an up-to-date review of galaxy formation and evolution and its future prospects.

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7.

Low-metallicity Star Formation (IAU S255):From the First Stars to Dwarf Galaxies

作者：Leslie K. Hunt 出版社：Cambridge Univ Pr 出版日：2009/02/23 裝訂：精裝

Although low-mass metal-poor galaxies in the local universe have often been proposed as the 'primordial building blocks' in the hierarchical scenario of structure formation, several lines of evidence suggest that this may not be true. Moreover, it is not clear to what extent dwarf galaxies, because they are metal poor and because of their kinematics and structure, can tell us about how star formation proceeded in the early universe. This volume provides an overview and the most recent advances in this debate. IAU Symposium 255 presents the most up-to-date developments in six key areas, including: Population III and metal-free star formation; metal-enrichment, chemical evolution and feedback; explosive events in low-metallicity environments; dust and gas as seeds for metal-poor star formation; metal-poor initial mass functions, stellar evolution and star-formation histories; and low-metallicity star formation in the local universe. This overview is at a level suitable for research astro

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8.

Dwarf Galaxies Iau S344 ― From the Deep Universe to the Present

作者：Kristen B. W. McQuinn 出版社：Cambridge Univ Pr 出版日：2019/08/31 裝訂：精裝

Dwarf galaxies are important tools for understanding structure formation and galaxy evolution across cosmic time. These low-mass systems allow us to gain a detailed understanding of stellar, chemical, and dynamical properties in the nearby universe; they also provide a unique window into the complex physics of the early universe. The Proceedings of IAU Symposium 344 present our current understanding of dwarf galaxies, with sections dedicated to: Local Group dwarf galaxies; the interstellar medium and star formation in dwarfs; metallicity, massive stars, and chemical evolution; the dwarf galaxy–environment connection; low-mass galaxies at high redshift; and dwarfs as cosmological probes. Broad overviews from leaders in the field, detailed presentation of cutting-edge results, and short summaries of a wide range of work are included for each of these topics, suitable for both experts and newcomers to the field.

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9.

Why Galaxies Care About Agb Stars ― A Continuing Challenge Through Cosmic Time

作者：Franz Kerschbaum 出版社：Cambridge Univ Pr 出版日：2019/09/30 裝訂：精裝

Stars on the asymptotic giant branch (AGB stars) play an important role due to their high luminosity and production of heavy elements and cosmic dust. They are prime laboratories for studying situations where different physical and chemical processes work simultaneously, on different time scales. IAU Symposium 343 builds a bridge between research on AGB stars themselves and their applications to the modelling of stellar populations and the chemical evolution of galaxies. Our understanding of these complex stars is given using insights into many aspects of physics and chemistry, while very high-angular resolution observations of AGB stars and their surroundings provide strong constraints on stellar theory and how they lose matter through strong stellar winds. This volume also highlights the difficulties in estimating the importance of AGB stars for various aspects of galaxies. Current developments and challenges of these complex objects are discussed for a broad, interdisciplinary audie

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90折

10.

Galaxies：Structure and Evolution

作者：Roger John Tayler 出版社：Cambridge Univ Pr 出版日：1993/03/04 裝訂：平裝

Galaxies are large systems of stars, some of which contain interstellar gas and dust. They also contain much invisible matter, which may be in the form of weakly interacting elementary particles. In this introductory textbook, the first chapter introduces the study of galaxies. This is followed by two chapters on observations of galaxies, including our own. There are then three chapters on galactic structure: the manner in which motions of stars determine galactic shape, the determination of galactic masses, and the structure of discs in spirals. Galactic evolution, especially changes in chemical composition over time, is covered. The book concludes with a discussion of the origin of galaxies and their relation to more general questions in cosmology. The book includes mathematical presentation where this enables the discussion to be quantitative.

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定價：2599 元，優惠價：9 2339

11.

Chemical Abundances in the Universe (IAU S265):Connecting First Stars to Planets

作者：Katia Cunha 出版社：Cambridge Univ Pr 出版日：2010/04/26 裝訂：精裝

IAU Symposium 265 presents a unified picture of nucleosynthesis, the production of chemical elements over cosmic time. It explains how this chemical evolution links together the early Universe of the first stars, through the formation of galaxies and their diverse populations of stars, to a Universe of heavy-element rich stars and planets. The first generation of massive stars that drove reionization left their chemical signatures imprinted in the oldest low-mass stars, which we observe today. Chemical evolution is a broad, diverse and rapidly evolving field, due to the ever-expanding capabilities delivered by new arrays of instruments on large telescopes, together with significant advances in modelling and increasing access to large and accurate nuclear, atomic, and molecular databases. Written for researchers and graduate students, the topics covered in this volume provide a comprehensive overview of the scientific progress achieved in recent years.

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12.

Galaxy Evolution across the Hubble Time (IAU S235)

作者：Françoise Combes 出版社：Cambridge Univ Pr 出版日：2007/05/17 裝訂：精裝

This last decade has witnessed a revolution in our observations of galaxies; in particular deep imaging with HST and spectroscopy with 10m-class ground-based telescopes have uncovered many objects that are difficult to place along the Hubble sequence. High resolution spectroscopy of extremely faint objects has enabled the study of the kinematic evolution and, hence, the mass assembly of galaxies to unprecedented look-back times for direct comparison with cosmological structure formation scenarios. Thus, it is now possible to study all three aspects of galaxy evolution - their morphological-dynamical, chemical and spectral evolution out to redshift larger than six, exploring more than 95% of the age of the universe. These Proceedings of the IAU Symposium 235 report the considerable progress made in recent years on galaxy formation and evolution, and look forward to the expected breakthroughs in the domain of remote galaxies, with ALMA, the ELT and the next generation space telescopes.

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13.

The General Assembly of Galaxy Halos, Iau S317 ― Structure, Origin and Evolution

作者：Angela Bragaglia 出版社：Cambridge Univ Pr 出版日：2016/07/01 裝訂：精裝

The proceedings of IAU S317 offer an updated view of the stellar halos of galaxies, from the local universe to more distant systems, discussing differences and similarities among them. They review the results of ongoing large photometric and spectroscopic surveys and compare them to the predictions of new generation simulations at the forefront of our technical capabilities. Structures are analysed on both large and small scales, with attention given to the kinematical and chemical properties of their smallest and oldest components. A number of excellent reviews on state-of-the-art research, covering fields such as first stars, galactic archaeology, stellar halos in cosmological simulations, discrete constituents of stellar halos - from field, isolated stars to globular clusters and planetary nebulae - are accompanied by contributed papers presenting the results of original research by top-level specialists in the area. IAU S317 benefits researchers with interests encompassing stellar

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14.

Cosmochemistry：The Melting Pot of the Elements

作者：C. Esteban 出版社：Cambridge Univ Pr 出版日：2004/03/18 裝訂：精裝

The chemical composition of the Universe has evolved over billions of years. A host of astrophysical processes and observations must be understood in order to explain why celestial objects have the chemical compositions observed. Originally published in 2004, this book contains the lectures delivered at the XIII Canary Islands Winter School of Astrophysics, which was dedicated to reviewing current knowledge about the origin and evolution of the chemical elements in the Universe. Written by seven prestigious astrophysics researchers, it covers cosmological and stellar nucleosynthesis, abundance determinations in stars and ionised nebulae, chemical composition of nearby and distant galaxies, and models of chemical evolution of galaxies and intracluster medium. This is a timely review of developments in cosmochemistry over the last decade.

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15.

The Formation of the Milky Way

作者：E. J. Alfaro 出版社：Cambridge Univ Pr 出版日：1995/08/03 裝訂：精裝

Is the current state of our Galaxy primarily the result of its initial conditions or is it the product of a lifetime of complex interactions with its environment? Gathered in this volume are papers presented at an international meeting in Granada, Spain, dedicated to exploring this fundamental question. This review examines all the key physical processes involved in the formation and evolution of the Milky Way. A dozen invited review articles by international experts summarise our understanding to date; whilst more than seventy topical research papers present the latest results. Together, these papers provide a view on topical issues such as disk instabilities, large-scale star formation, large-scale structure formation in our Galaxy, chemical evolution, Disk-Halo feedback, the galactic globular cluster system, stellar populations, and the formation of galaxies. Also included are three panel sessions identifying key routes for critical future research.

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90折

16.

Cosmochemistry:The Melting Pot of the Elements

作者：C. Esteban 出版社：Cambridge Univ Pr 出版日：2010/09/09 裝訂：平裝

The chemical composition of the Universe has evolved over billions of years. A host of astrophysical processes and observations must be understood in order to explain why celestial objects have the chemical compositions observed. Originally published in 2004, this book contains the lectures delivered at the XIII Canary Islands Winter School of Astrophysics, which was dedicated to reviewing current knowledge about the origin and evolution of the chemical elements in the Universe. Written by seven prestigious astrophysics researchers, it covers cosmological and stellar nucleosynthesis, abundance determinations in stars and ionised nebulae, chemical composition of nearby and distant galaxies, and models of chemical evolution of galaxies and intracluster medium. This is a timely review of developments in cosmochemistry over the last decade.

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定價：2534 元，優惠價：9 2281

90折

17.

The Formation of the Milky Way

作者：E. J. Alfaro 出版社：Cambridge Univ Pr 出版日：2010/09/30 裝訂：平裝

Is the current state of our Galaxy primarily the result of its initial conditions or is it the product of a lifetime of complex interactions with its environment? Gathered in this volume are papers presented at an international meeting in Granada, Spain, dedicated to exploring this fundamental question. This review examines all the key physical processes involved in the formation and evolution of the Milky Way. A dozen invited review articles by international experts summarise our understanding to date; whilst more than seventy topical research papers present the latest results. Together, these papers provide a view on topical issues such as disk instabilities, large-scale star formation, large-scale structure formation in our Galaxy, chemical evolution, Disk-Halo feedback, the galactic globular cluster system, stellar populations, and the formation of galaxies. Also included are three panel sessions identifying key routes for critical future research.

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定價：2274 元，優惠價：9 2047

18.

The Lives and Death-throes of Massive Stars - Iau S329

作者：J.J. Eldridge 出版社：Cambridge Univ Pr 出版日：2017/06/30 裝訂：精裝

Research on massive stars is undergoing a period of rapid progress, with long-held convictions being shown to be incomplete. While these stars are relatively few in number, they are the main driver of chemical and dynamical evolution in galaxies through their stellar winds and explosive deaths in core-collapse supernovae. Furthermore the impact of massive stars is widely recognized in many areas, as they are often used as tools to interpret the conditions and processes arising in different environments. In parallel, the development of new instrumentation, analysis techniques and dedicated surveys across all possible wavelengths have delivered large amounts of exquisite new data. These data are now providing a harsh test for the current state-of-the-art theoretical calculations of massive star birth, evolution and death. IAU Symposium 329 covers these topics and is therefore an invaluable resource for researchers in the field of massive stars and their evolution.

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Stellar Astrophysics for the Local Group:VIII Canary Islands Winter School of Astrophysics

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19.

Stellar Astrophysics for the Local Group:VIII Canary Islands Winter School of Astrophysics

作者：A. Aparicio 出版社：Cambridge Univ Pr 出版日：2010/09/30 裝訂：平裝

With the advent of large, ground-based telescopes and space telescopes, it is now possible to study in detail stars outside our galaxy - in neighbouring galaxies in the so-called Local Group. The VIII Canary Islands Winter School of Astrophysics gathered leading experts from around the world to review this exciting area of research - extragalactic stellar astrophysics. This volume presents eight specially written articles based on the meeting, reviewing how the study of stars in nearby galaxies can be used to understand stellar and galactic structure and evolution in general. This book covers all aspects of extragalactic stellar astrophysics: stellar physics, stellar winds, stellar evolution, the use of photometric and spectroscopic techniques for studying extragalactic stars, stellar populations, chemical evolution, star formation histories and the calibration of the extragalactic distance scale. This volume provides graduate students and researchers with an invaluable introduction to

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定價：3314 元，優惠價：9 2983

20.

STELLAR POPULATIONS

作者：RENZINI 出版社：JOHN WILEY & SONS;LTD 出版日：2011/09/21 裝訂：精裝

This only up-to-date reference on stellar populations and development models includes coverage of distant galaxies, chemical evolution and supernovae. Written by highly acclaimed authorities in the fi

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