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原文書 (26)
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可訂購商品 (26)
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無庫存 (26)
商品定價

$800以上 (26)
出版日期

2024年 (8)
2022~2023 (8)
2020~2021 (10)
裝訂方式

精裝 (26)
作者

;Bonifacio, Piercarlo (l'Observatoire de Paris, France),Cioni, Maria-Rosa (Leibniz-Institut fur Astrophysik, Potsdam),Hammer, Francois (l'Observatoire de Paris, France),Pawlowski, Marcel S. (Leibniz-I (1)
;Mackey, Jonathan (Dublin Institute for Advanced Studies),Vink, Jorick S. (Armagh Observatory),St-Louis, Nicole (Universite de Montreal) (1)
;Wong, Tony (University of Illinois Urbana-Champaign),Kim, Woong-Tae (Seoul National University) (1)
Alessandra Celletti (1)
Alexander G. Kosovichev (1)
Angela Bragaglia (1)
Dmitry Bisikalo (1)
Elisabete da Cunha (1)
Leen Decin (1)
Maria Teresa Lago (1)
Martin A. Barstow (1)
Mirjana Pović (1)
Monica Valluri (1)
Médéric Boquien (1)
Rosa M. Ros (1)
Thaisa Storchi Bergmann (1)
Troja, Eleonora (NASA-Goddard Space Flight Center),Baring, Matthew (Rice University, Houston) (1)
;Cauzzi, Gianna (National Solar Observatory, USA),Tritschler, Alexandra (National Solar Observatory, USA) (1)
;Elmegreen, Debra (Vassar College, New York) (1)
;Hirota, Tomoya (National Astronomical Observatory of Japan, Japan),Imai, Hiroshi (Kagoshima University, Japan),Pihlstrom, Ylva (University of New Mexico),Menten, Karl (Max-Planck-Institut fur Radioas (1)
出版社/品牌

Cambridge Univ Pr (13)
Cambridge University Press (13)

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26筆商品,1/2頁
Massive Stars Near and Far (IAU S361)
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02-25006600[分機130、131]。
Resolving the Rise and Fall of Star Formation in Galaxies (IAU S373)
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02-25006600[分機130、131]。
The Origin of Outflows in Evolved Stars (IAU S366)
作者:Leen Decin  出版社:Cambridge Univ Pr  出版日:2022/09/30 裝訂:精裝
The prime parameter determining the evolution of a star is its mass. Any modification to the stellar mass has large repercussions on its evolutionary path. Both low-mass and massive stars are known to power strong stellar winds at the end of their lives. These winds determine the type of the stellar end product and the amount by which these stars contribute to the chemical enrichment of the interstellar medium, ultimately providing the building blocks of planets and life. A proper understanding of stellar evolution and the building blocks in the Universe cannot be achieved without a detailed understanding of stellar winds. IAU Symposium 366 provides an overview of state-of-the-art observational and theoretical studies on the origin of winds in low-mass and massive evolved stars, with topics including binarity, enrichment of the interstellar medium, astrochemistry, and theoretical, observational and numerical constraints on stellar outflows.
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02-25006600[分機130、131]。
The Predictive Power of Computational Astrophysics as a Discovery Tool (IAU S362)
作者:Dmitry Bisikalo  出版社:Cambridge Univ Pr  出版日:2022/09/30 裝訂:精裝
A new paradigm for scientific discovery through computational tools now permeates every aspect of astronomical research. Computational astrophysics combines modern computational methods, novel hardware designs, advanced algorithms, original software implementations, and associated technologies to discover new phenomena and to make predictions in astronomy. The proceedings of IAU Symposium 362 summarizes ongoing developments in computational astrophysics through astronomers in diverse fields sharing their knowledge and approaches. It focuses on computational methods applied to speed up and broaden the scope of scientific studies, such as finding trends in observational data, high performance computing, automated search algorithms, and model predictability. Experts discuss a palette of challenging informational and technical developments, with the goal of coordinating their efforts and the improvement of techniques in pursuit of a wide range of astronomical studies, including fluid
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02-25006600[分機130、131]。
The Era of Multi-Messenger Solar Physics (IAU S372)
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02-25006600[分機130、131]。
Multi-scale (Time and Mass) Dynamics of Space Objects (IAU S364)
作者:Alessandra Celletti  出版社:Cambridge Univ Pr  出版日:2022/06/30 裝訂:精裝
The range of phenomena that manifest at all different time and length scales and the wide range of sizes of space objects, from minor bodies in the Solar System to exoplanets, and from dust particles to Jupiter-size bodies, require the development of dynamical modeling and analysis tools that can handle these different scales. This volume collects contributions given by distinguished scientists at the hybrid IAU Symposium 364. The methods in dynamics modeling of space objects have already reached a state of maturity, and their implementation provided a large number of important results pertaining to both the theory and their applications. The contributions cover the recent advances in the multi-scale dynamics of natural and artificial space objects from various perspectives, which will benefit graduate students and researchers working in the fields of celestial mechanics, astrodynamics, planetary sciences, applied mathematics and dynamical systems.
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02-25006600[分機130、131]。
Galaxy Evolution and Feedback across Different Environments (IAU S359)
作者:Thaisa Storchi Bergmann  出版社:Cambridge Univ Pr  出版日:2020/12/31 裝訂:精裝
The goal of IAU Symposium 359 on 'Galaxy Evolution and Feedback across Different Environments' (GALFEED) was to bring together the active galactic nuclei (AGN) and galaxy evolution scientific communities. The AGN phase occurs in most galaxies and critically influences their evolution, so it is important to study the two processes together and for researchers, in both topics, to learn from one another. They ask key questions such as: How do galaxies acquire their gas and how efficiently is it transformed into stars? How is the supermassive black hole in a galaxy center fuelled to become an AGN? What is the main physical mechanism that quenches star formation? How powerful are the stellar and AGN feedback processes in regulating galaxy evolution? And what is the role of the environment on galaxy evolution and AGN triggering? Astronomers engage in these discussions spanning from early galaxies to the present day.
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02-25006600[分機130、131]。
Education and Heritage in the Era of Big Data in Astronomy (IAU S367):The First Steps on the IAU 2020-2030 Strategic Plan
作者:Rosa M. Ros  出版社:Cambridge Univ Pr  出版日:2021/10/31 裝訂:精裝
For thousands of years people have looked to the skies to better understand the universe and our place within it. Crucially it is the role of teachers and experts to make astronomical concepts accessible to the next generation, and to pass on our collective knowledge for others to build on. This volume brings together contributions from modern pioneers in astronomy education, as presented at the online IAU Symposium 367 on 'Education and Heritage in the Era of Big Data in Astronomy'. Topics covered include cultural astronomy and heritage, technological advances, citizen science, inclusivity initiatives, interdisciplinary science education and open astronomy. Particular focus is given to how emerging technologies provide new opportunities to connect with budding astronomers. Many of the techniques discussed can be applied by educators at different levels and in a range of settings, from school classrooms and lecture halls to informal public spaces such as museums and planetariums.
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02-25006600[分機130、131]。
Proceedings of the Thirtieth General Assembly Vienna 2018:IAU Transactions XXX
作者:Elmegreen; Debra (Vassar College; New York)  出版社:Cambridge University Press  出版日:2024/03/31 裝訂:精裝
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02-25006600[分機130、131]。
Uncovering Early Galaxy Evolution in the ALMA and JWST Era (IAU S352)
作者:Elisabete da Cunha  出版社:Cambridge Univ Pr  出版日:2020/05/31 裝訂:精裝
The first three billion years of cosmic time were the prime epoch of galaxy formation. Characterising galaxies at this epoch is therefore crucial to achieving a major goal of modern astrophysics: to understand how galaxies such as our Milky Way emerged from the primordial density fluctuations in the early Universe and how they evolved through cosmic time. Recent major international investments in observing facilities such as the Atacama Large Millimetre Array (ALMA) and the James Webb Space Telescope (JWST) promise to provide the next leap in our understanding of this topic. This volume gathers the scientific contributions to the International Astronomical Union Symposium 352, which was devoted to this topic. The community of theoretical and observational experts discuss how we can make the most of ALMA and JWST synergies in advancing our understanding of galaxy evolution in the young Universe.
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02-25006600[分機130、131]。
Galactic Dynamics in the Era of Large Surveys (IAU S353)
作者:Monica Valluri  出版社:Cambridge Univ Pr  出版日:2020/05/31 裝訂:精裝
Galactic dynamics is fundamental to understanding the formation of galaxies, their internal evolution and their current structure. While galactic dynamics has traditionally focused on the evolution of the stellar components of galaxies, studies over the past two decades have shown that all aspects of galaxy evolution are strongly influenced by the interplay between the dynamics of stars, gas, and dark matter. IAU Symposium 353, is the first major symposium in more than a decade focused on the dynamics of galaxies and stellar systems, covering the recent explosion in the availability of kinematical data both for individual stars in the Milky Way and wide field line-of-sight kinematics for large samples of external galaxies. These proceedings describe recent developments that aim to transform our understanding of the dynamics, structure, formation and evolution of our own host galaxy, the Milky Way, as well as galaxies in the universe at large.
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02-25006600[分機130、131]。
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