LEADER 02726nam 2200373 450 001 9910669802903321 005 20230513231941.0 035 $a(CKB)5710000000111628 035 $a(NjHacI)995710000000111628 035 $a(EXLCZ)995710000000111628 100 $a20230513d2019 uy 0 101 0 $aeng 135 $aur||||||||||| 181 $ctxt$2rdacontent 182 $cc$2rdamedia 183 $acr$2rdacarrier 200 10$aFundamentals of galaxy dynamics, formation and evolution /$fIgnacio Ferreras 210 1$aLondon :$cUCL Press,$d2019. 215 $a1 online resource (xvi, 181 pages) $cillustrations 311 $a1-911307-66-5 327 $a1. An introduction to galaxy formation -- 2. The classical theory of gravitation -- 3. A statistical treatment of stellar systems -- 4. Understanding our Galaxy -- 5. Specific aspects of disc and elliptical galaxies -- 6. Galactic chemical enrichment -- 7. The growth of density fluctuations -- 8. Smaller stellar systems: Stellar clusters -- 9. Larger stellar systems: Galaxy clusters. 330 $aGalaxies, along with their underlying dark matter halos, constitute the building blocks of structure in the Universe. Of all fundamental forces, gravity is the dominant one that drives the evolution of structures from small density seeds at early times to the galaxies we see today. The interactions among myriads of stars, or dark matter particles, in a gravitating structure produce a system with fascinating connotations to thermodynamics, with some analogies and some fundamental differences. Ignacio Ferreras presents a concise introduction to extragalactic astrophysics, with emphasis on stellar dynamics, and the growth of density fluctuations in an expanding Universe. Additional chapters are devoted to smaller systems (stellar clusters) and larger ones (galaxy clusters). Fundamentals of Galaxy Dynamics, Formation and Evolution is written for advanced undergraduates and beginning postgraduate students, providing a useful tool to get up to speed in a starting research career. Some of the derivations for the most important results are presented in detail to enable students appreciate the beauty of maths as a tool to understand the workings of galaxies. Each chapter includes a set of problems to help the student advance with the material. 606 $aGalaxies$xEvolution 606 $aGalaxies$xFormation 615 0$aGalaxies$xEvolution. 615 0$aGalaxies$xFormation. 676 $a523.112 700 $aFerreras$b Ignacio$0862445 801 0$bNjHacI 801 1$bNjHacl 906 $aBOOK 912 $a9910669802903321 996 $aFundamentals of Galaxy Dynamics, Formation and Evolution$91925165 997 $aUNINA LEADER 03266oam 2200493I 450 001 9910149367903321 005 20240501153258.0 010 $a1-315-35440-3 010 $a1-315-37163-4 010 $a1-4987-0551-0 024 7 $a10.4324/9781315371634 035 $a(CKB)3710000000933743 035 $a(MiAaPQ)EBC4732199 035 $a(OCoLC)960707123 035 $a(BIP)68889173 035 $a(BIP)52306953 035 $a(EXLCZ)993710000000933743 100 $a20180331h20172017 uy 0 101 0 $aeng 135 $aurcnu|||||||| 181 $ctxt$2rdacontent 182 $cc$2rdamedia 183 $acr$2rdacarrier 200 10$aDistrict cooling $etheory and practice /$fAlaa A. Olama 205 $a1st ed. 210 1$aBoca Raton :$cCRC Press,$d[2017] 210 4$dİ2017 215 $a1 online resource (127 pages) $cillustrations, tables 225 1 $aHeat transfer : a series of reference books and textbooks 311 08$a1-4987-0550-2 320 $aIncludes bibliographical references and index. 327 $achapter 1. Introduction to district cooling -- chapter 2. Economic considerations -- chapter 3. Major factors influencing the design of a district cooling system -- chapter 4. Designing central plants -- chapter 5. Designing chilled water distribution systems -- chapter 6. Designing energy transfer stations -- chapter 7. Design of thermal energy storage -- chapter 8. Controls and instrumentation. 330 $aDISTRICT COOLING: THEORY and PRACTICE provides a unique study of an energy cogeneration system, set up to bring chilled water to buildings (offices, apartment houses, and factories) needing cooling for air conditioning and refrigeration. In winter, the source for the cooling can often be sea water, so it is a cheaper resource than using electricity to run compressors for cooling. The related technology of District Heating has been an established engineering practice for many years, but District Cooling is a relatively new technology now being implemented in various parts of the world, including the USA, Arab Emirates and Kuwait, and Saudi Arabia. Existing books in the area are scarce, and do not address many of the crucial issues facing nations with high overall air temperatures, many of which are developing District Cooling plans using sea water. DISTRICT COOLING: THEORY & PRACTICE integrates the theory behind district cooling planning with the practical engineering approaches, so it can serve the policy makers, engineers, and planners whose efforts have to be coordinated and closely managed to make such systems effective and affordable. In times of rising worldwide temperatures, District Cooling is a way to provide needed cooling with energy conservation and sustainability. This book will be the most up-to-date and comprehensive study on the subject, with Case Studies describing real projects in detail. 410 0$aHeat transfer (Boca Raton, Fla.) 606 $aAir conditioning from central stations 615 0$aAir conditioning from central stations. 676 $a697.9/3 700 $aOlama$b Alaa A.$0905117 801 0$bFlBoTFG 801 1$bFlBoTFG 906 $aBOOK 912 $a9910149367903321 996 $aDistrict cooling$92024383 997 $aUNINA