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Protostars and Planets V by Bo Reipurth,David Jewitt,Klaus Keil Pdf
'Protostars and Planets V' builds on the latest results from recent advances in ground and space-based astronomy and in numerical computing techniques to offer the most detailed and up-to-date picture of star and planet formation - including the formation and early evolution of our own solar system.
Henrik Beuther,Ralf S. Klessen,Cornelis Petrus Dullemond,Thomas K. Henning
Author : Henrik Beuther,Ralf S. Klessen,Cornelis Petrus Dullemond,Thomas K. Henning Publisher : University of Arizona Press Page : 945 pages File Size : 44,8 Mb Release : 2014-12-18 Category : Science ISBN : 9780816531240
Protostars and Planets IV by Vincent Mannings,Alan Boss,Sara Samantha Russell Pdf
Click here for the online version of this book! This title, out of print in 2008, is now available free of charge, in it's entirety, online through the University of Arizona Press! Both a textbook and a status report for every facet of research into the formation of stars and planets, Protostars and Planets IV brings together 167 authors who report on the most significant advances in the field since the publication of the previous volume in 1993. Protostars and Planets IV reflects improvements in observational techniques and the availability of new facilities such as the Infrared Space Observatory, the refurbished Hubble Space Telescope, and the 10-m Keck telescopes. Advances in computer technology and modeling methods have benefited theoretical studies of molecular clouds, star formation, and jets and disks, while recent analyses of meteorites yield important insights into conditions and processes within our Sun's early protoplanetary disk. The 49 chapters describe context and progress for observational and theoretical studies of the structure, chemistry, and dynamics of molecular clouds; the collapse of cores and the formation of protostars; the formation and properties of young binary stars; the properties of winds, jets, and molecular outflows from young stellar objects; the evolution of circumstellar envelopes and disks; grain growth in disks and the formation of planets; and the properties of the early Solar nebula. Protostars and Planets IV is also the first book to include chapters describing the discoveries of extrasolar planets, brown dwarfs, and Edgeworth-Kuiper Belt objects, and the first to include high-resolution optical and near-infrared images of protoplanetary disks. Protostars and Planets IV is an unsurpassed reference not only for established researchers but also for younger scientists whose imagination and work will lead to tomorrow's discoveries.
Protostellar Jets in Context by Kanaris Tsinganos,Tom Ray,Matthias Stute Pdf
It is over a quarter of a century since the discovery of out?ows from young stars. The intervening years have led to remarkable advances in our understanding of this phenomenon. Much of the progress can be attributed to advances in facilities and technologies, including not only larger telescopes but also improved instrument and detector performance. In addition protostellar out?ows have now been imaged from the ground and space at high spatial resolution, e. g. with HST, and at a wide - riety of wavelengths from X-rays to radio waves, revealing more and more about their physics. This veritable revolution in observation has been accompanied by an exponential growth in our ability to numerically simulate the launching and pro- gation of jets. Codes continue to improve: they now incorporate more physics and are increasingly ef?cient through, for example, techniques such as adaptive mesh re?nement and the use of parallel processing in cluster environments. Simulating the launching and propagation of a jet all the way from the vicinity of the star up to 4 several thousand AU (a size range of10 ) is now much closer. In more recent times, developments in observation, theory and numerical s- ulation have been joined by laboratory jet experiments reproducing, on centimetre scales, that which is seen in astrophysics to stretch for several parsecs.
Advances in Geosciences is the result of a concerted effort to bring together the latest results and planning activities related to earth and space science in Asia and the international arena. The volume editors are all leading scientists in their research fields covering six sections: Atmospheric Science (AS), Hydrological Science (HS), Ocean Science (OS), Solid Earth (SE), Solar Terrestrial (ST) and Planetary Science (PS). The main purpose is to highlight the scientific issues essential to the study of earthquakes, tsunamis, atmospheric dust storms, climate change, drought, flood, typhoons, monsoons, space weather, and planetary exploration. This volume is abstracted in NASA's Astrophysics Data System: http://ads.harvard.edu Contents:Volume 10: Atmospheric Science (AS) Rainfall over Thailand during ENSO (1997–2000) (Wonlee & Prungchan)Formation of Tropical Cyclone Concentric Eye Walls by Wave–Mean Flow Interactions (J-Y Peng et al.)Anthropogenic Aerosol Radiative Forcing in the INDO-Gangetic Basi (S Dey & S N Tripathi)and other papersVolume 11: Hydrological Science (HS)Study for the Fresh Ground Water Resources, Neil, Island, India (V K Saxena)Emerging Concepts in Hydrology for Tropical Pacific Regimes (J Terry)Analysis of Monami Waves in Aquatic Vegetation (S Patil et al.)and other papersVolume 12: Ocean Science (OS)3D Current Characteristics Simulation with ANN (C Z Chew et al.)Classification of Ocean Waves from the Data Buoy Measurements (R Balaji et al.)Intercomparison of Various Latent Heat Flux Products in the South China Sea (Zhen et al.)and other papersVolume 13: Solid Earth (SE)The International Laser Ranging Service (M Pearlman et al.)Numerical Modeling of the 2006 Java Tsunami Earthquake (N R Hanifa et al.)Statistical Properties and Time Trend in the Number of Holocene Volcanic Eruptions. (A N Zemtsov & A A Tron)and other papersVolume 14: Solar Terrestrial (ST)ULF Waves: Exploring the Earth's Magnetosphere (B J Fraser)Spectrum of Density Fluctuations in the Solar Wind (V Krishnan)Polarization Properties of the Ultra-Low Frequency Waves in Non-Axisymmetric Background Magnetic Fields (K Kabin et al.)and other papersVolume 15: Planetary Science (PS)X-Rays from Nonmagnetic Planets (K Dennerl)Clouds, Clumps, Cores, and Comets — A Cosmic Chemical Connection? (S B Charnley & S D Rodgers)Comparative X-Ray Studies of Planetary Aurorae (G Branduardi-Raymont)and other papers Readership: Academics, researchers and postgraduate students in geosciences. Key Features: Provides an important source of new and not-yet-published results from the growing Asian and international geoscience community Presents a unique view of the rapid scientific progress made by Asian researchers in topics crucial to the future of the global environment Highlights a first-hand description of how the largest scientific population in the world is working together to manage the environmental problems which will determine the economic and social growth of the world itselfKeywords:Planetary Science;Atmosphere;Ionosphere;Magnetosphere “This set is the result of an effort to bring together the latest results and planning activities related to earth and space science in Asia and the international arena. The main purpose of this set is to highlight the scientific issues essential to the study of earthquakes, tsunami, atmospheric dust storms, climate change, drought, floods, typhoons, monsoons, space weather, and planetary exploration.” Bulletin of the American Meteorological Society
Advances in Geosciences is the result of a concerted effort to bring together the latest results and planning activities related to earth and space science in Asia and the international arena. The volume editors are all leading scientists in their research fields covering six sections: Atmospheric Science (AS), Hydrological Science (HS), Ocean Science (OS), Solid Earth (SE), Solar Terrestrial (ST) and Planetary Science (PS). The main purpose is to highlight the scientific issues essential to the study of earthquakes, tsunamis, atmospheric dust storms, climate change, drought, flood, typhoons, monsoons, space weather, and planetary exploration. This volume is abstracted in NASA''s Astrophysics Data System: http: //ads.harvard.edu. Contents: X-Rays from Nonmagnetic Planets (K Dennerl); Clouds, Clumps, Cores, and Comets OCo A Cosmic Chemical Connection? (S B Charnley & S D Rodgers); Comparative X-Ray Studies of Planetary Aurorae (G Branduardi-Raymont); and other papers. Readership: Academics, researchers and postgraduate students in geosciences."
Turbulence and Self-Organization by Mikhail Ya Marov,Aleksander V. Kolesnichenko Pdf
The book deals with the development of continual models of turbulent natural media. Such models serve as a ground for the statement and numerical evaluation of the key problems of the structure and evolution of the numerous astrophysical and geophysical objects. The processes of ordering (self-organization) in an originally chaotic turbulent medium are addressed and treated in detail with the use of irreversible thermodynamics and stochastic dynamics approaches which underlie the respective models. Different examples of ordering set up in the natural environment and outer space are brought and thoroughly discussed, the main focus being given to the protoplanetary discs formation and evolution.
Planets in Binary Star Systems by Nader Haghighipour Pdf
In 1988, in an article on the analysis of the measurements of the variations in the radial velocities of a number of stars, Campbell, Walker, and Yang reported an - teresting phenomenon;the radial velocity variations of Cephei seemed to suggest the existence of a Jupiter-like planet around this star. This was a very exciting and, at the same time, very surprising discovery. It was exciting because if true, it would have marked the detection of the ?rst planet outside of our solar system. It was surprising because the planet-hosting star is the primary of a binary system with a separation less than 19 AU, a distance comparable to the planetary distances in our solar system. The moderatelyclose orbit of the stellar companionof Cephei raised questions about the reality of its planet. The skepticism over the interpretation of the results (which was primarily based on the idea that binary star systems with small sepa- tions would not be favorable places for planet formation) became so strong that in a subsequent paper in 1992, Walker and his colleagues suggested that the planet in the Cephei binary might not be real, and the variations in the radial velocity of this star might have been due to its chromospheric activities.
Triggered Star Formation in a Turbulent Interstellar Medium (IAU S237) by International Astronomical Union. Symposium Pdf
New stars form in the dense turbulent gas clouds of galaxies, and the formation of these clouds is the subject of the IAU S237. This book is the most up-to-date review of all aspects of cloud and star formation, and one of the few compendiums available on ISM turbulence.
Author : Paulo J. V. Garcia Publisher : University of Chicago Press Page : 437 pages File Size : 41,5 Mb Release : 2011-05-15 Category : Science ISBN : 9780226282299
Physical Processes in Circumstellar Disks Around Young Stars by Paulo J. V. Garcia Pdf
Circumstellar disks are vast expanses of dust that form around new stars in the earliest stages of their birth. Predicted by astronomers as early as the eighteenth century, they weren’t observed until the late twentieth century, when interstellar imaging technology enabled us to see nascent stars hundreds of light years away. Since then, circumstellar disks have become an area of intense study among astrophysicists, largely because they are thought to be the forerunners of planetary systems like our own—the possible birthplaces of planets. This volume brings together a team of leading experts to distill the most up-to-date knowledge of circumstellar disks into a clear introductory volume. Understanding circumstellar disks requires a broad range of scientific knowledge, including chemical processes, the properties of dust and gases, hydrodynamics and magnetohydrodynamics, radiation transfer, and stellar evolution—all of which are covered in this comprehensive work, which will be indispensable for graduate students, seasoned researchers, or even advanced undergrads setting out on the study of planetary evolution.
Protostars & Planets by Tom Gehrels,Mildred Shapley Matthews Pdf
Unique source book on star formation and the origin of planetary systems from some 35 distinguished authors. Topics include the formation of stars from the cloudy to the stellar to the planetary state. Special emphasis on stars believed capable of producing planets.
