Galaxies and stars Books
David Chandler Company Cardboard Night Sky Planisphere Southern
Book Synopsis
£9.95
Clarendon Press The Mathematical Theory of Black Holes
Book SynopsisPart of the reissued Oxford Classic Texts in the Physical Sciences series, this book was first published in 1983, and has swiftly become one of the great modern classics of relativity theory. It represents a personal testament to the work of the author, who spent several years writing and working-out the entire subject matter.The theory of black holes is the most simple and beautiful consequence of Einstein''s relativity theory. At the time of writing there was no physical evidence for the existence of these objects, therefore all that Professor Chandrasekhar used for their construction were modern mathematical concepts of space and time. Since that time a growing body of evidence has pointed to the truth of Professor Chandrasekhar''s findings, and the wisdom contained in this book has become fully evident.Trade ReviewThere is no doubt in my mind that this book is a masterpiece...beautifully written and well-presented. * Roger Penrose in Nature *"Chandrasekhar has provided us with a magisterial text on the classical black holes, outstanding in the depth and detail of its coverage...Throughout, a wealth of mathematical ideas is explained and employed in the process of extracting the properties of these space-times, and the similarities and differences between the different black hole space-times are thoroughly treated. This book is an undoubted classic, and wil remain a standard reference work on black holes for many years." Mathematics Today, October 1999Table of Contents1. Mathematical preliminaries ; 2. A space-time of sufficient generality ; 3. The Schwarzchild space-time ; 4. The perturbations of the Schwarzchild black hole ; 5. The Reissner-Nordstrom solution ; 6. The Kerr metric ; 7. The geodesics in the Kerr space-time ; 8. Electromagnetic waves in Kerr geometry ; 9. The gravitational perturbations of the Kerr black hole ; 10. Spin-1/2 particles in Kerr geometry ; 11. Other solutions ; 12. Other methods
£85.50
Yale University Press The Realm of the Nebulae
Book SynopsisIn less than a century, the accepted picture of the universe transformed from a stagnant place, comprised entirely of our own Milky Way galaxy, to a realm inhabited by billions of individual galaxies, hurtling away from one another. In this title, the author describes his principal observations and conclusions.Trade Review"This enduring work is the closest we can get to Edwin Hubble’s personal thoughts as he broke open the boundaries of the universe in the early twentieth century. In this compelling summary of his historic observations of myriad galaxies swiftly moving outward in space-time, we see both his awe—and his doubts—over the new and surprising cosmos he had revealed. A true classic of scientific literature."—Marcia Bartusiak, MIT, author of The Day We Found the Universe -- Marcia Bartusiak
£32.67
Springer Galactic Bulges
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£151.65
Springer Planetary Nebulae
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£156.75
Springer Pulsation Rotation and Mass Loss in EarlyType Stars
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£143.62
Springer Co
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£201.49
Springer Galaxy Evolution
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£143.62
Cambridge University Press Philosophy of Cosmology and Astrophysics
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£55.00
Creative Media Partners, LLC Summary Report for Concentrating Solar Power Thermal Storage Workshop
£21.80
Creative Media Partners, LLC Summary Report for Concentrating Solar Power Thermal Storage Workshop
£13.22
Cambridge University Press Stellar Structure and Evolution
Book SynopsisThis textbook for upper-level undergraduate and graduate students in astronomy aims to develop a physical understanding of the fundamental principles that dictate stellar properties. Focusing on key physical processes without going into encyclopedic depth, the authors explain the life cycle of stars in a broad contemporary context.Trade Review'Pinsonneault and Ryden's book is a very welcome addition to the field of stellar evolution at a level appropriate to advanced undergraduate- or graduate-level study, since it manages to provide a clear, comprehensive overview of topics, without being intimidating in size or style. The textbook includes up-to-date results from contemporary missions such as Gaia and Kepler, with the final chapters discussing stellar rotation, pulsations, and binary evolution in depth. Most chapters include a few well-designed exercises, with a research-level reading list provided after the appendix. I would highly recommend it for Master's-level courses on stellar structure and evolution.' Paul Crowther, University of Sheffield'This text is a welcome addition to the pantheon of monographs and textbooks explaining the physical basics of stellar structure and evolution. Aimed primarily at an audience learning the material for the first time, this text explains the phases of the life of a star through a clear application of physical principles. Weaving together classical fluids, quantum mechanics, thermodynamics, and nuclear physics, it enables students and their instructors to gain the physical intuition needed for the study of stars in this time of their observational renaissance.' Lars Bildsten, University of California, Santa Barbara'This is a welcome addition to the literature, providing a comprehensive overview of stellar structure and evolution, and including insights from the latest data, techniques, and results.' William Chaplin, University of BirminghamTable of ContentsPreface; 1. Properties of stars; 2. Equations of stellar structure; 3. Equations of state; 4. Stellar energy transport; 5. Stars as fusion reactors; 6. Main sequence stars; 7. Star formation: before the main sequence; 8. Evolved stars: after the main sequence; 9. Ex-stars; 10. Rotating stars; 11. Pulsating stars; 12. Binary stars; Appendices; Bibliography, references, and figure credits; Index.
£39.99
Sacred Light Publishing The Grand Solar Flash: The Event of a Lifetime
£27.47
The University of Chicago Press HighEnergy Radiation from Magnetized Neutron
Book SynopsisNeutron stars, the most extreme state of matter yet confirmed, are responsible for much of the high-energy radiation detected in the universe. Meszaros provides a general overview of the physics of magnetized neutron stars, discusses in detail the radiation processes and transport properties relevant to the production and propagation of high-energy radiation in the outer layers of these objects, and reviews the observational properties and theoretical models of various types of neutron star sources.
£72.20
The University of Chicago Press Black Holes and Relativistic Stars
Book SynopsisBlack holes and neutron stars are generally recognized as key components of many astrophysical systems. Based on a symposium held in honour of S. Chandrasekhar, these papers provide a comprehensive summary of progress made in the 1990s on the theory of black holes and relativistic stars.Table of ContentsContributors Preface 1: Gravitational Waves, Stars and Black Holes Valeria Ferrari 2: Rotating Relativistic Stars John L. Friedman 3: Probing Black Holes and Relativistic Stars with Gravitational Waves Kip S. Thorne 4: Astrophysical Evidence for Black Holes Martin J. Rees 5: The Question of Cosmic Censorship Roger Penrose 6: Black Hole Collisions, Toroidal Black Holes, and Numerical Relativity Saul A. Teukolsky 7: The Internal Structure of Black Holes Werner Israel 8: Black Holes and Thermodynamics Robert M. Wald 9: The Statistical Mechanics of Black Hole Thermodynamics Rafael D. Sorkin 10: Generalized Quantum Theory in Evaporating Black Hole Spacetimes James B. Hartle 11: Is Information Lost in Black Holes? Stephen W. Hawking 12: Quantum States of Black Holes Gary T. Horowitz Chandra: A Tribute Kameshwar C. Wali Our Song Lalitha Chandrasekhar
£76.00
University of Arizona Press Protostars and Planets VI
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£52.50
University of Hawai'i Press North Star to Southern Cross
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£16.11
Johns Hopkins University Press Things That Go Bump in the Universe
Book SynopsisExperience the drama of the explosive cosmos and the astonishing discoveries being made about the universe's wildest phenomena. The violent birth of the universe was only the first bang of a very bumpy ride. This unfathomably cacophonous beginning has spawned blasts, implosions, cosmic cannibalism, collisions, and countless other fleeting energetic events punctuating the cosmos. Although often brief, these transient phenomena pack a powerful punch. Armed with decades of theoretical progress, unrivaled computing power, and cutting-edge technology, astronomers find themselves at the cusp of understanding not just the events themselves, but also how those events reveal the story of the entire cosmos. In Things That Go Bump in the Universe, astronomer and science writer C. Renée James introduces us to her colleagues around the world, who are using pioneering research techniques to explore everything from the very first explosions in the universe to the dark energy that could destroy it aTrade ReviewLike a pulsar, the book is at times dense, but it also dazzles. It recasts modern astronomy as the search for transient, explosive events, and the messages they contain if only we can decode them.—New York Times Book ReviewTable of ContentsPrologue. Flashes of InsightChapter 1. Catching Cosmic FirefliesChapter 2. Out of the QuestionChapter 3. Putting the "Super" in SupernovaChapter 4. Star-Shattering EnergyChapter 5. The Search for Smoking GunsChapter 6. Detecting Cosmic HeartbeatsChapter 7. Stellar ArrhythmiaChapter 8. (Almost) No Star Is an IslandChapter 9. The Making of a SuperstarChapter 10. Cloudy with a Chance of NeutrinosChapter 11. Not "The End"Chapter 12. Collision CourseChapter 13. Fallen StarsChapter 14. Don't BlinkChapter 15. Point BlankChapter 16. Cats, Rats, and Fantastic Beasts, and How to Tell Them Apart Chapter 17. Cosmic TremorsChapter 18. The Return of the FurbiesChapter 19. LIGO, We Have a ProblemChapter 20. Impeccable TimingChapter 21. All Together NowChapter 22. Multiple Eyewitness AccountsChapter 23. Furbies—A New HopeChapter 24. The First Bumps in the Universe Chapter 25. The Last HurrahEpilogue. EphemeraAcknowledgmentsBibliographyIndex
£22.50
Chelsea House Publishers Edward Pickering and His Women Computers: Analyzing the Stars
£29.71
Reaktion Books Galaxy Mapping the Cosmos
Book SynopsisWritten by an active researcher in the field, Galaxy: Mapping the Cosmos tells the rich scientific story of galaxy evolution and observation. Appealing to all readers interested in astronomy and cosmology, and featuring 100 colour illustrations, Galaxy explores the enigma of our cosmic habitat, chronicling how our home in the universe came to be.
£23.38
ISTE Ltd Galaxies: Formation and Evolution
Book SynopsisGalaxies are vast ensembles of stars, gas and dust, embedded in dark matter halos. They are the basic building blocks of the Universe, gathered in groups, clusters and super-clusters. They exist in many forms, either as spheroids or disks. Classifications, such as the Hubble sequence (based on mass concentration and gas fraction) and the colormagnitude diagram (which separates a blue cloud from a red sequence) help to understand their formation and evolution. Galaxies spend a large part of their lives in the blue cloud, forming stars as spiral or dwarf galaxies. Then, via a mechanism that is still unclear, they stop forming stars and quietly end in the red sequence, as spheroids. This transformation may be due to galaxy interactions, or because of the feedback of active nuclei, through the energy released by their central super-massive black holes. These mechanisms could explain the history of cosmic star formation, the rate of which was far greater in the first half of the Universe�s life. Galaxies delves into all of these surrounding subjects in six chapters written by dedicated, specialist astronomers and researchers in the field, from their numerical simulations to their evolutions.Table of ContentsIntroduction xi Chapter 1. The Classification of Galaxies 1Ronald BUTA 1.1. Introduction 1 1.2. Classes of galaxies 3 1.3. Elliptical galaxies 7 1.4. Spiral galaxies 12 1.5. S0 galaxies 22 1.6. Magellanic spiral and irregular galaxies 25 1.7. Dwarf elliptical, S0, and spheroidal galaxies 26 1.8. Edge-on galaxies 27 1.9. Morphology of interacting and merging galaxies 30 1.10. General properties along the CVRHS sequence 31 1.10.1. Morphological systematics 31 1.10.2. Astrophysical systematics 33 1.11. Other approaches to galaxy classification 34 1.12. Interpretations of morphology 35 1.13. Artificial galaxies and the future of galaxy classification 42 1.14. References 44 Chapter 2. Our Galaxy, the Milky Way 49Paola Di MATTEO 2.1. Introduction 49 2.2. Baryonic discs and their spiral structure 52 2.2.1. Neutral, ionized and molecular gas 52 2.2.2. Thin and thick stellar discs 54 2.2.3. Spiral structure from gaseous and stellar tracers 59 2.3. The central kiloparsecs: the bar and the bulge 60 2.4. The stellar halo 63 2.5. On the dark matter content and shape, as inferred from rotation curves and stellar streams 67 2.6. Dissecting the global structure: stellar kinematics, abundances and ages 69 2.6.1. Setting the scene: the solar vicinity 70 2.6.2. Zooming out on a several kpc scale 76 2.6.3. Digging into the bulge 80 2.7. Reconstructing the Milky Way evolution 84 2.8. Perspectives 86 2.9. References 86 Chapter 3. Early-type Galaxies 93Eric EMSELLEM 3.1. Introduction 93 3.2. General properties: components and morphology 95 3.2.1. Discs and bars 96 3.2.2. Gas and dust content 96 3.2.3. Dark matter and halo 97 3.2.4. Globular clusters 99 3.2.5. Light and mass profiles 99 3.2.6. Extreme cases: brightest cluster galaxies and ultra-diffuse galaxies 100 3.3. Zoom on the stellar component 101 3.3.1. Scaling relations: Faber–Jackson, fundamental plane and virial plane 102 3.3.2. Age and metallicity 104 3.3.3. Initial mass function 105 3.4. Dynamics of ETGs 108 3.4.1. Observations 109 3.4.2. Toward a kinematic classification of ETGs 110 3.4.3. Modeling 113 3.4.4. Supermassive black holes 119 3.5. Formation and evolution processes 119 3.5.1. Perspective at z = 0: the mass–radius plane 119 3.5.2. Growth, mergers and transformations 121 3.5.3. Ex situ versus in situ 123 3.5.4. Environment 124 3.6. Conclusion 126 3.7. References 127 Chapter 4. Spiral Galaxies 137Françoise COMBES 4.1. Introduction 137 4.2. Blue and red galaxies: quenching star formation 142 4.2.1. Definition of bimodality 142 4.2.2. The parameters that determine the red sequence 146 4.2.3. Mechanisms for quenching star formation 148 4.3. Spiral galaxies: density waves or not? 152 4.3.1. The winding problem 152 4.3.2. The theory of density waves 155 4.3.3. Role of gas and star formation 159 4.4. Bars: drivers of evolution 160 4.4.1. Formation of bars 162 4.4.2. Orbits in a barred galaxy 164 4.4.3. Response of gas to a barred potential 166 4.4.4. Vertical resonances and peanuts 168 4.4.5. Dark matter and bars 171 4.5. Environment of spiral galaxies 173 4.5.1. Morphological segregation 173 4.5.2. The problem of bulgeless galaxies 174 4.6. Conclusion 176 4.7. References 177 Chapter 5. Galaxy Mergers and Interactions through Cosmic Time 181Christopher J. CONSELICE 5.1. Introduction 182 5.2. The physics of merging 185 5.3. The merger history of galaxies 188 5.3.1. Defining mergers and merging 188 5.3.2. Merger rates in the nearby universe 190 5.3.3. Galaxy merger fraction evolution to z = 6 191 5.3.4. Galaxy merger rates 196 5.4. The added value of mergers 199 5.4.1. Galaxy and black hole assembly through interactions and mergers 199 5.4.2. Cosmological relevance 201 5.4.3. Future uses and methods 202 5.5. Summary 203 5.6. Acknowledgments 204 5.7. References 205 Chapter 6. Cosmic Evolution of Galaxies 209David ELBAZ and Emeric Le FLOC’H 6.1. Introduction 209 6.2. Characteristics of galaxies used to define their cosmic evolution 211 6.2.1. Decoding multi-wavelength radiation 211 6.2.2. Populations of galaxies 216 6.3. Starbursts, secular evolution and universality of star formation 218 6.3.1. Definition of a starburst 218 6.3.2. The SFMS and the secular evolution of galaxies 220 6.3.3. Origin of starbursts 221 6.3.4. Secular evolution and the influence of the galactic environment 223 6.4. Detection of distant galaxies 225 6.4.1. Deep surveys of the Universe 227 6.4.2. Large samples of distant galaxies 229 6.4.3. K correction 232 6.5. Cosmic history of galaxies 234 6.5.1. History of star formation 234 6.5.2. Evolution of the stellar mass function and formation of the red galaxy sequence 237 6.5.3. Evolution of the metallicity and of the average size of galaxies 239 6.5.4. Evolution of the galaxy merger and starburst rates 241 6.6. Origin of the cosmic history of galaxies 244 6.6.1. The diffuse cosmic background as a signature of the cosmic history of galaxies 245 6.6.2. Unraveling the origin of the cosmic history of galaxies by studying their reservoirs of interstellar matter 249 6.7. Conclusion 251 6.8. References 252 List of Authors 257 Author Biographies 259 Index 261
£124.15
Taylor & Francis Ltd AgeDating Stars
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£45.99
Taylor & Francis Ltd AgeDating Stars From the Sun to Distant Galaxies
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£114.00
Cambridge University Press Light Curves of Variable Stars
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£45.59
Cambridge University Press The Milky Way Galaxy and Statistical Cosmology 18901924
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Cambridge University Press Supernova 1987a in the Large Magellanic Cloud
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£44.64
Cambridge University Press Warped Disks and Inclined Rings Around Galaxies
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£35.14
Cambridge University Press Physics of the Pulsar Magnetosphere
Book SynopsisThis book presents the theory of the electrodynamic phenomena which occur in the magnetosphere of a pulsar. It also provides a clear picture of the formation and evolution of neutron stars. The authors address the basic physical processes of electron-positron plasma production, the generation of electric fields and currents, and the emission of radio waves and gamma rays. The book also reviews observational data, and devotes a complete chapter to a detailed comparison of this data with accepted theory and with some recent theoretical predictions. Tables containing the values of the physical parameters of all observed radio pulsars are also provided. The book is illustrated throughout and is fully referenced. Graduate students and researchers in astrophysics and plasma physics working in the field of radio pulsars will find this book of great value.Trade Review'I hope that other plasma physicists will take up the story; if they do, they should start with this seminal work.' The Observatory'… accessible for students in their 3rd year and also researchers in astrophysics and plasma physics.' La Recherche'… an important contribution to the literature and will be an essential addition to the libraries of all those active in either observations or modeling of pulsars.' American Review of ScienceTable of ContentsIntroduction; List of notation; Constants and quantities; 1. Basic observational characteristics of radio pulsars; 2. Neutron stars; 3. Physical processes in the pulsar magnetosphere; 4. Electrodynamics of the pulsar magnetosphere; 5. Generation of electron-positron plasma in the pulsar magnetosphere; 6. Pulsar radio emission; 7. Comparison of theory with observational data; Conclusion; Appendix; References; Additional literature; Author index; Subject index.
£39.89
Cambridge University Press Stellar Rotation 36 Cambridge Astrophysics Series Number 36
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£40.84
Cambridge University Press Origin Evolution Planetary Nebulae 33 Cambridge Astrophysics Series Number 33
Book SynopsisThis 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.Trade Review'… an accessible account of the origin and evolution of these enigmatic shells of gas. the generous, colourful images are the best feature of the book, but the text reveals the speedy evolution of ideas - matching the increase in data - in this complex field, as a microcosm of the way in which modern astronomy is developing.' Astronomy & Geophysics'The book addresses three aspects of planetary nebula (PN) research: radiation mechanisms and PN evolution and the associated spin-offs in laboratory spectroscopy. Kwok's book is now the standard reference.' Irish Astronomical Journal'This book presents a thoroughly modern understanding of planetary nebulae, integrating new developments in stellar physics with the dynamics of nebular evolution.' Europe & Astronomy'… a valuable contribution … It offers the most complete and accessible entry to this subject for the newcomer with a strong general background in physics and astronomy at the advanced undergraduate level or above.' Physics Today'… it was a sheer pleasure to read this new book by Sun Kwok. The book is slim and stylish, characteristic of the Cambridge Astrophysics Series.' Dr X.-W. Lou, Contemporary PhysicsTranslation: 'In sum, The Origin and Evolution of Planetary Nebulae is a technical book undeniably rich demonstrations, quantitative data and mathematical formulas, which is primarily intended for researchers and graduate students in astronomy and astrophysics.' Yves Laberge, Physics in CanadaTable of ContentsPreface; 1. History and overview; 2. Ionization structure of planetary nebulae; 3. Nebular line radiation; 4. Nebular continuum radiation; 5. The neutral gas component; 6. The dust component; 7. Observations of the central star of planetary nebulae; 8. Morphologies of planetary nebulae; 9. Problems and questions; 10. Asymptotic giant branch stars - progenitors of planetary nebulae; 11. Evolution of the central stars; 12. Formation of planetary nebulae; 13. Dynamical evolution of planetary nebulae; 14. Proto-planetary nebulae - the transition objects; 15. Evolution to the white dwarf stage; 16. Distances to planetary nebulae; 17. Comparison between evolutionary models and observations; 18. PN in the galactic context; 19. Chemical abundances; 20. Planetary nebulae in other galaxies; 21. Concluding remarks; References; Appendix: list of symbols and abbreviations; Subject index.
£51.29
Cambridge University Press Stellar Astrophysical Fluid Dynamics
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Cambridge University Press Messiers Nebulae and Star Clusters
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Cambridge University Press Globular Cluster Systems 30 Cambridge Astrophysics Series Number 30
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Cambridge University Press In Darkness Born
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Cambridge University Press Coevolution of Black Holes and Galaxies
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Cambridge University Press Clusters of Galaxies Probes of Cosmological Structure and Galaxy Volume 3 Carnegie Observatories Astrophysics 4 Volume Paperback Set
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Cambridge University Press Extrasolar Planets Canary Islands Winter School of Astrophysics
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Cambridge University Press Extreme Stars
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Cambridge University Press Compact Stellar Xray Sources 39 Cambridge Astrophysics Series Number 39
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Cambridge University Press The Formation of the Milky Way
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Cambridge University Press Hot Stars in the Galactic Halo
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Cambridge University Press The Local Group as an Astrophysical Laboratory Proceedings of the Space Telescope Science Institute Symposium held in Baltimore Maryland May 58 Institute Symposium Series Series Number 17
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Cambridge University Press Supernovae
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Cambridge University Press AGN Feedback in Galaxy Formation Cambridge Contemporary Astrophysics
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Cambridge University Press Active OB Stars IAU S272 Structure Evolution MassLoss and Critical Limits Proceedings of the International Astronomical Union Symposia and Colloquia
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Cambridge University Press Understanding Variable Stars Cambridge Astrophysics
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Cambridge University Press The Milky Way Galaxy and Statistical Cosmology 18901924
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Cambridge University Press Quasars Redshifts and Controversies
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