The Spectral Energy Distribution of Galaxies - SED 2011 (IAU S284) PDF Download
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Author: Richard J. Tuffs
Publisher: Cambridge University Press
ISBN: 9781107019843
Category : Science
Languages : en
Pages : 533
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Book Description
Recent observational developments are providing the first truly panchromatic view of galaxies, extending from the radio to TeV gamma-rays. This is motivating the development of new models for the interpretation of spectral energy distributions (SEDs) of galaxies in terms of the formation, evolution and emission of stellar and accretion-driven sources of photons, the interaction of the photons with the gaseous and dust components of the interstellar medium, and high-energy processes involving cosmic rays. IAU Symposium 284 details progress in the development of such models, their relation to fundamental theory, and their application to the interpretation of the panchromatic emission from the Milky Way and nearby galaxies, connecting the latter with models for the evolution of the SEDs of distant galaxies, and the extragalactic background light. IAU S284 is a useful resource for all researchers working with the copious amounts of multiwavelength data for galaxies now becoming available.
Author: Richard J. Tuffs
Publisher: Cambridge University Press
ISBN: 9781107019843
Category : Science
Languages : en
Pages : 533
Get Book Here
Book Description
Recent observational developments are providing the first truly panchromatic view of galaxies, extending from the radio to TeV gamma-rays. This is motivating the development of new models for the interpretation of spectral energy distributions (SEDs) of galaxies in terms of the formation, evolution and emission of stellar and accretion-driven sources of photons, the interaction of the photons with the gaseous and dust components of the interstellar medium, and high-energy processes involving cosmic rays. IAU Symposium 284 details progress in the development of such models, their relation to fundamental theory, and their application to the interpretation of the panchromatic emission from the Milky Way and nearby galaxies, connecting the latter with models for the evolution of the SEDs of distant galaxies, and the extragalactic background light. IAU S284 is a useful resource for all researchers working with the copious amounts of multiwavelength data for galaxies now becoming available.
Author: Evangelos Simoudis
Publisher:
ISBN:
Category : Computers
Languages : en
Pages : 414
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Book Description
Author: Loukas Vlahos
Publisher: Springer Science & Business Media
ISBN: 3642002099
Category : Science
Languages : en
Pages : 332
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Book Description
Over the years, many leading European graduate schools in the field of astrophysical and space plasmas have operated within the framework of the research network, "Theory, Observations, and Simulations in Turbulence in Space Plasmas." This text is a set of lectures and tutorial reviews culled from the relevant work of all those schools. It emphasizes applications on solar coronae, solar flares, and the solar wind. In bridging the gap between standard textbook material and state-of-the-art research, this text offers a broad flavor to postgraduate and postdoctoral students just coming to the field. And because of its unique mix, it will also be useful to lecturers looking for advanced teaching material for their seminars and courses.
Author: Harry Edward Payne
Publisher:
ISBN:
Category : Astronomy
Languages : en
Pages : 568
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Book Description
Author: Cristina C. Popescu
Publisher: American Institute of Physics
ISBN:
Category : Science
Languages : en
Pages : 492
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Book Description
Heidelberg, Germany, 4-8 October 2004
Author: Shuanggen Jin
Publisher: CRC Press
ISBN: 1482214881
Category : Science
Languages : en
Pages : 399
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Book Description
Although lunar exploration began in the 1960s, the moon and other planets have many long-standing, unanswered questions about planetary environments, origin, formation and evolution, magnetization of crustal rocks, internal structure, and possible life. However, with the recent development of planetary geodesy and remote sensing with higher spatial and spectral resolution have come new opportunities to explore and understand the moon and planets in greater detail. Written by well-established, international scientists in the planetary science and remote sensing fields, Planetary Geodesy and Remote Sensing presents the latest methods and techniques of planetary geodesy and remote sensing. The book discusses the latest results in planetary science, including theory, methods, measurements, topography, gravity and magnetic field, atmosphere and ionosphere, geomorphology, volcano, craters, internal structure, and water. The book also highlights comparative studies with the earth in the atmosphere, geomorphology, and interiors of the planets. It discusses future missions and future objectives of planetary exploration and science using the latest advances in remote sensing. With chapters contributed by a stellar list of pioneers and experts, the book provides new insight on the application of new technologies and the observations in planetary geodesy. It is suitable for those working in the field as well as for planetary probe designers, engineers, and planetary geologists and geophysicists.
