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1. |
Record Nr. |
UNINA9910700881103321 |
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Titolo |
DCFUEL submission quick start guide version 0.1 [[electronic resource]] |
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Pubbl/distr/stampa |
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[Washington, D.C.] : , : Compliance and Innovative Strategies Division, Office of Transportation and Air Quality, U.S. Environmental Protection Agency, , [2011] |
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Edizione |
[Version 0.1.] |
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Descrizione fisica |
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1 online resource (13 pages) : color illustrations |
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Soggetti |
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Motor fuels - United States - Quality control - Computer programs |
Electronic data interchange |
Quality assurance |
Standardization |
Forms management |
Motor fuels - United States |
Handbooks and manuals. |
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Lingua di pubblicazione |
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Formato |
Materiale a stampa |
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Livello bibliografico |
Monografia |
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Note generali |
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Title from title screen (viewed on Aug. 15, 2011). |
"EPA420-B-11-029." |
"July 2011." |
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2. |
Record Nr. |
UNINA9910796617403321 |
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Autore |
Zhang Xiaolei |
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Titolo |
Dynamical evolution of galaxies / / Ziaolei Zhang |
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Pubbl/distr/stampa |
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Berlin ; ; Boston : , : De Gruyter, , [2018] |
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©2018 |
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ISBN |
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Descrizione fisica |
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1 online resource (338 pages) |
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Disciplina |
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Soggetti |
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Galaxies - Evolution |
Nucleosynthesis |
Milky Way |
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Lingua di pubblicazione |
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Formato |
Materiale a stampa |
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Livello bibliografico |
Monografia |
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Nota di bibliografia |
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Includes bibliographical references and index. |
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Nota di contenuto |
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Frontmatter -- Preface -- Contents -- 1. Introduction -- 2. Dynamical Drivers of Galaxy Evolution -- 3. N-Body Simulations of Galaxy Evolution -- 4. Astrophysical Implications of the Dynamical Theory -- 5. Putting It All Together -- 6. Concluding Remarks -- 7. Appendix: Relation to Kinetics and Fluid Mechanics -- References -- Index |
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Sommario/riassunto |
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This research monograph presents a new dynamical framework for the study of secular morphological evolution of galaxies along the Hubble sequence. Classical approaches based on Boltzmann's kinetic equation, as well as on its moment-equation descendants the Euler and Navier-Stokes fluid equations, are inadequate for treating the maintenance and long-term evolution of systems containing self-organized structures such as galactic density-wave modes. A global and synthetic approach, incorporating correlated fluctuations of the constituent particles during a nonequilibrium phase transition, is adopted to supplement the continuum treatment. The cutting-edge research combining analytical, N-body simulational, and observational aspects, as well as the fundamental-physics connections it provides, make this work a valuable reference for researchers and graduate students in astronomy, astrophysics, cosmology, many-body physics, complexity theory, and other related fields. ContentsDynamical Drivers of Galaxy EvolutionN-Body Simulations of Galaxy EvolutionAstrophysical Implications of the |
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Dynamical TheoryPutting It All TogetherConcluding RemarksAppendix: Relation to Kinetics and Fluid Mechanics |
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