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 #  AuthorTitleAccn#YearItem Type Claims
161 Raymond Lyttleton The stability of rotating liquid masses OB0633 Book  
162 edited by Robert Williams, Mario Livio The analysis of emission lines OB0632 Book  
163 Andrea Milani and Giovanni F. Gronchi Theory of orbit determination OB0631 Book  
164 Peter R. Wilson Solar and stellar activity cycles OB0630 Book  
165 edited by David G. Blair The detection of gravitational waves OB0629 Book  
166 James Jeans Through Space and Time OB0628 Book  
167 Annamaneni Peraiah An introduction to radiative transfer OB0627 Book  
168 edited by Michael F. Bode, Aneurin Evans Classical novae OB0626 Book  
169 edited by G. Tenorio-Tagle Violent star formation from 30 Doradus to QSOs OB0625 Book  
170 Re??mi Hakim An introduction to relativistic gravitation OB0624 Book  
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161.    
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TitleThe stability of rotating liquid masses
Author(s)Raymond Lyttleton
EditionFirst paperback edition
Description1 online resource (150 pages) : digital, PDF file(s)
Abstract NoteRaymond Arthur Lyttleton (1911???95) was a British astronomer who won the Royal Society Royal Medal in 1965 for significant contributions to his field. In this book, which was first published in 1953, Lyttleton presents an account of advances in relation to a classical problem of mathematical astronomy. The text is mainly concerned with those parts of the theory most directly involved in determining the evolution of gravitating liquid masses. The important conclusion is reached that the dynamical evidence is against the so-called 'fission process' of binary system formation. This book will be of value to anyone with an interest in astronomy and the history of science
NotesTitle from publisher's bibliographic system (viewed on 06 Jun 2016)
Keyword(s)1. EBOOK 2. EBOOK - CAMBRIDGE UNIVERSITY PRESS 3. ROTATING MASSES OF FLUID 4. STABILITY
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162.     
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TitleThe analysis of emission lines : a meeting in honour of the 70th birthdays of D.E. Osterbrock & M.J. Seaton : proceedings of the Space Telescope Science Institute Symposium, held in Baltimore, Maryland, May 16-18, 1994
Author(s)edited by Robert Williams, Mario Livio
Description1 online resource (xi, 223 pages) : digital, PDF file(s)
Abstract NoteWhat can emission lines tell us about an astrophysical object? A workshop at the Space Telescope Science Institute was dedicated to address just this question ??? for a host of objects (including planetary nebulae and active galactic nuclei) across a broad range of wavelengths (from the infrared through to gamma-rays). Thirteen review articles from internationally renowned experts are presented in this volume. They provide an edited and coherent overview of the latest technical data, techniques in and applications of the study of emission lines from a variety of objects. Chapters include the theory of radiative transfer, photoionising shocks, and emission lines from stellar winds, as well as useful summaries of abundance determinations, atomic data, and diagnostics for IR, UV, gamma-ray and molecular lines. Together these review articles provide an overview of the analysis of emission lines. They summarise current knowledge, highlight outstanding problems and provide focus for fruitful future research. In this way they provide an excellent introduction for graduate students and reference for professionals
NotesTitle from publisher's bibliographic system (viewed on 05 Oct 2015)
Keyword(s)1. ASTRONOMICAL SPECTROSCOPY 2. EBOOK 3. EBOOK - CAMBRIDGE UNIVERSITY PRESS 4. EMISSION SPECTROSCOPY
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163.     
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TitleTheory of orbit determination
Author(s)Andrea Milani and Giovanni F. Gronchi
Description1 online resource (x, 382 pages) : digital, PDF file(s)
Abstract NoteDetermining orbits for natural and artificial celestial bodies is an essential step in the exploration and understanding of the Solar System. However, recent progress in the quality and quantity of data from astronomical observations and spacecraft tracking has generated orbit determination problems which cannot be handled by classical algorithms. This book presents new algorithms capable of handling the millions of bodies which could be observed by next generation surveys, and which can fully exploit tracking data with state-of-the-art levels of accuracy. After a general mathematical background and summary of classical algorithms, the new algorithms are introduced using the latest mathematical tools and results, to which the authors have personally contributed. Case studies based on actual astronomical surveys and space missions are provided, with applications of these new methods. Intended for graduate students and researchers in applied mathematics, physics, astronomy and aerospace engineering, this book is also of interest to non-professional astronomers
Contents NotePreface -- Part I. Problem Statement and Requirements -- 1. The problem of orbit determination -- 2. Dynamical systems -- 3. Error models -- 4. The N-body problem -- Part II. Basic Theory -- 5. Least squares -- 6. Rank deficiency -- Part III. Population Orbit Determination -- 7. The identification problem -- 8. Linkage -- 9. Methods by Laplace and Gauss -- 10. Weakly determined orbits -- 11. Surveys -- 12. Impact monitoring -- Part IV. Collaborative Orbit Determination -- 13. The gravity of a planet -- 14. Non-gravitational perturbations -- 15. Multi arc strategy -- 16. Satellite gravimetry -- 17. Orbiters around other planets -- References -- Index
NotesTitle from publisher's bibliographic system (viewed on 05 Oct 2015)
Keyword(s)1. CELESTIAL MECHANICS 2. EBOOK 3. EBOOK - CAMBRIDGE UNIVERSITY PRESS 4. ORBIT DETERMINATION
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164.     
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TitleSolar and stellar activity cycles
Author(s)Peter R. Wilson
Description1 online resource (xviii, 274 pages) : digital, PDF file(s)
Abstract NoteHow do you predict the parameters of future solar cycles? What is the role of dynamo theory in the cyclic activity of the Sun and similar stars? And what are the implications of chaos theory for stellar cycles? This book answers these questions and offers a timely review of studies in the cyclic activity of the Sun and other stars. This authoritative reference shows the importance of reliable predictions of the parameters of future solar cycles, and carefully explains the methods currently used to determine these (with special reference to the maximum of cycle 22). Some of the latest research into solar cycles is clearly presented; this includes helioseismology, observations of the extended activity cycle and the polar fields reversal, and contributions from dynamo theory and chaos theory. For graduate students and researchers, this monograph provides a much-needed synthesis of our understanding of activity cycles in the Sun and other stars
Contents Note1. Introduction. 1.1. The significance of stellar activity cycles. 1.2. The solar-stellar connection. 1.3. The solar cycle and the terrestrial environment -- 2. Historical survey. 2.1. The discovery of sunspots. 2.2. The Maunder Minimum. 2.3. The periodicity law. 2.4. The Carrington rotation and the solar flare. 2.5. The Zurich sunspot number. 2.6. Latitude drift and the butterfly diagram. 2.7. The Wilson effect. 2.8. Hale and the Mount Wilson era. 2.9. The magnetic fields of sunspots. 2.10. The magnetic cycle. 2.11. The polar fields -- 3. The structure of the Sun and the phenomena of activity. 3.1. Basic data. 3.2. Radiative transfer. 3.3. The limb darkening. 3.4. Departures from spherical symmetry. 3.5. The chromosphere and the corona. 3.6. The chromospheric structures. 3.7. Prominences. 3.8. Flares. 3.9. Coronal structures. 3.10. Coronal holes. 3.11. Active longitudes -- 4. The equations of magnetohydrodynamics and magnetohydrostatics. 4.1. Maxwell's equations and the induction equation
NotesTitle from publisher's bibliographic system (viewed on 05 Oct 2015)
Keyword(s)1. ASTROPHYSICS 2. EBOOK 3. EBOOK - CAMBRIDGE UNIVERSITY PRESS 4. SOLAR CYCLE 5. STARS
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OB0630     On Shelf    

165.     
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TitleThe detection of gravitational waves
Author(s)edited by David G. Blair
Description1 online resource (xxiv, 481 pages) : digital, PDF file(s)
Abstract NoteGravitational radiation has not been positively detected. Over the past two decades an army of extremely sensitive detectors has been built up, so that today its detection appears inevitable. In the opening chapters of this 1991 book David Blair introduces the concepts of gravitational waves within the context of general relativity. The sources of gravitational radiation for which there is direct observational evidence and those of a more speculative nature are described. He then gives a general introduction to the methods of detection. In the subsequent chapters he has drawn together the leading scientists in the field to give a comprehensive practical and theoretical account of the physics and technology of gravitational wave detection. David Blair has extensive knowledge of the subject and has visited most of the gravitational radiation experiments over the world. He has compiled a book which will be of lasting value to specialists, both the postgraduates and researchers in the field
NotesTitle from publisher's bibliographic system (viewed on 05 Oct 2015)
Keyword(s)1. EBOOK 2. EBOOK - CAMBRIDGE UNIVERSITY PRESS 3. GRAVITATIONAL WAVES
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166.     
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TitleThrough Space and Time
Author(s)James Jeans
Description1 online resource (300 pages) : digital, PDF file(s)
Abstract NoteThrough Space and Time is based upon the 1933 Christmas Lectures that James Jeans gave at the Royal Institution, London. Intended to appeal to a wide readership and presenting a broad understanding of the Earth, solar system and the universe, the book begins its journey with the history, structure and main features of our planet, and ends in the vast expanses of space among the nebulae
NotesTitle from publisher's bibliographic system (viewed on 05 Oct 2015)
Keyword(s)1. EBOOK 2. EBOOK - CAMBRIDGE UNIVERSITY PRESS
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OB0628     On Shelf    

167.     
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TitleAn introduction to radiative transfer : methods and applications in astrophysics
Author(s)Annamaneni Peraiah
Description1 online resource (xii, 480 pages) : digital, PDF file(s)
Abstract NoteAstrophysicists have developed several very different methodologies for solving the radiative transfer equation. An Introduction to Radiative Transfer presents these techniques as applied to stellar atmospheres, planetary nebulae, supernovae, and other objects with similar geometrical and physical conditions. Accurate methods, fast methods, probabilistic methods and approximate methods are all explained, including the latest and most advanced techniques. The book includes the different techniques used for computing line profiles, polarization due to resonance line scattering, polarization in magnetic media and similar phenomena. Exercises at the end of each chapter enable these methods to be put into practice, and enhance understanding of the subject. This 2001 book will be valuable to graduates, postgraduates and researchers in astrophysics
NotesTitle from publisher's bibliographic system (viewed on 05 Oct 2015)
Keyword(s)1. EBOOK 2. EBOOK - CAMBRIDGE UNIVERSITY PRESS 3. RADIATIVE TRANSFER 4. STARS
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OB0627     On Shelf    

168.     
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TitleClassical novae
Author(s)edited by Michael F. Bode, Aneurin Evans
EditionSecond edition
Description1 online resource (xxii, 375 pages) : digital, PDF file(s)
Abstract NoteThis second edition has been updated and revised and contains contributions covering important developments in this field, and reflecting on interesting insights into classical novae. The book examines thermonuclear processes, the evolution of nova systems, nova atmospheres and winds, the evolution of dust and molecules in novae, nova remnants and observations of novae in other galaxies. It includes observations across the electromagnetic spectrum, from radio to gamma rays, and discusses some of the most important outstanding problems in classical nova research
Contents NoteNovae : an historical perspective / Hilmar W. Duerbeck -- Properties of novae : an overview / Brian Warner -- The evolution of nova-producing binary stars / Icko Iben Jr. and Masayuki Y. Fujimoto -- Thermonuclear processes / Sumner Starrfield, Christian Iliadis, and W. Raphael Hix -- Nova atmospheres and winds / Peter H. Hauschildt -- Observational mysteries and theoretical challenges for abundance studies / Jordi Jose?? and Steven N. Shore -- Radio emission from novae / E.R. Seaquist and M.F. Bode -- Infrared studies of classical novae / Robert D. Gehrz -- Optical and ultraviolet evolution / Steven N. Shore -- X-ray emission from classical novae in outburst / Joachim Krautter -- Gamma-rays from classical novae / Margarita Hernanz -- Resolved nebular remnants / T.J. O'Brien and M.F. Bode -- Dust and molecules in nova environments / A. Evans and J.M.C. Rawlings -- Extragalactic novae / Allen W. Shafter
NotesTitle from publisher's bibliographic system (viewed on 05 Oct 2015)
Keyword(s)1. EBOOK 2. EBOOK - CAMBRIDGE UNIVERSITY PRESS 3. Stars, New
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OB0626     On Shelf    

169.     
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TitleViolent star formation from 30 Doradus to QSOs : proceedings of the first IAC-RGO meeting, held in Puerto Naos La Palma, Spain, November 8-12, 1993
Author(s)edited by G. Tenorio-Tagle
Description1 online resource (xiii, 431 pages) : digital, PDF file(s)
Abstract NoteWhat impact do massive stellar associations have on their environment through the power of their ionising radiation and mechanical energy? Gathered together in this volume are papers presented at the first IAC???RGO meeting, held in Puerto Naos La Palma, Spain, dedicated to exploring all aspects of this burning question. This volume examines the formation and evolution of new stellar clusters, and explores all the possible consequences in a wide variety of objects where massive stellar bursts have occurred. Thus it presents an alternative model to that of supermassive black holes as the power houses of active galactic nuclei; it analyses the impact of Wolf???Rayet stars, stellar winds and supernovae on their host galaxy; and it provides evidence of massive superassociations and of supersonic velocity dispersions which result from photo-ionisation by violent star formation. For graduate students and researchers, this volume provides a valuable overview and a timely update on all aspects of violent star formation in a host of objects - from 30 Doradus, the largest HII region in the Large Magellanic Cloud, to nuclear starbursts and QSOs
NotesTitle from publisher's bibliographic system (viewed on 05 Oct 2015)
Keyword(s)1. EBOOK 2. EBOOK - CAMBRIDGE UNIVERSITY PRESS 3. STARS
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OB0625     On Shelf    

170.    
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TitleAn introduction to relativistic gravitation
Author(s)Re??mi Hakim
Description1 online resource (ix, 271 pages) : digital, PDF file(s)
Abstract NoteThis is an introductory textbook on applications of general relativity to astrophysics and cosmology. The aim is to provide graduate students with a toolkit for understanding astronomical phenomena that involve velocities close to that of light or intense gravitational fields. The approach taken is first to give the reader a thorough grounding in special relativity, with space-time the central concept, following which general relativity presents few conceptual difficulties. Examples of relativistic gravitation in action are drawn from the astrophysical domain. The book can be read on two levels: first as an introductory fast-track course, and then as a detailed course reinforced by problems which illuminate technical examples. The book has extensive links to the literature of relativistic astrophysics and cosmology
NotesTitle from publisher's bibliographic system (viewed on 05 Oct 2015)
Keyword(s)1. ASTROPHYSICS 2. COSMOLOGY 3. EBOOK 4. EBOOK - CAMBRIDGE UNIVERSITY PRESS 5. GENERAL RELATIVITY (PHYSICS)
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