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- 要約等Galaxies are the fundamental units of cosmic matter ......p the universe and they change in...... billion years of cosmic time. W......iscovering how galaxies we can see ove......these billions of years are evol......, more massive and passive system......the structural evolution of galaxies, how we measur......nge with time, and how observing ......laxy formation and evolution. It also explains the future of the field through the use of machine learning tools, and how galaxy structure can be used as......nique features of the universe, ......cal properties and parameters
- 内容細目...lar, peculiar, and dwarf galaxies 1.4. Low surface brightness galaxies 1.5. Primer on galaxy structure and galaxy formation 1.6. Book structure 2. Galaxy structure and its meaning 2.......the properties of galaxies 2.2. A new cla......asuring galaxy structures 3.1. Parametr......c measurements of structure 3.2. Size meas......rgers 3.5. Non-evolutionary effects on structure 3.6. Summary 4......ual morphology evolution 4.4. Galaxy bar evolution 4.5. The formation of spiral structure 4.6. Numerical simulations of galaxy structure 5. Physical evolution of galaxy structure 5.1. Local uni...... morphological evolution 5.4. Morphological k-correcti...
- 件名Galaxies--Formation Galaxies--Evolution Galaxies--Évolution Galaxies & stars. SCIENCE--Astronomy. Galaxies--Evolution. Galaxies--Formation.
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- 出版者（掲載誌）Kyoto : Publication Office
デジタル記事
インターネットで読める国立国会図書館全国の図書館
- 出版者（掲載誌）Kyoto : Publication Office
デジタル記事
インターネットで読める国立国会図書館全国の図書館
- 出版者（掲載誌）Kyoto : Publication Office
デジタル記事
インターネットで読める国立国会図書館全国の図書館
- 出版者（掲載誌）Kyoto : Publication Office
デジタル記事
インターネットで読める国立国会図書館全国の図書館
- 出版者（掲載誌）Kyoto : Publication Office
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国立国会図書館全国の図書館
- 出版者（掲載誌）Kyoto : Publication Office
紙図書
国立国会図書館
- 内容細目Introduction and overview Therm......mic abundances of elements and isotopes Cosmo......ucleosynthesis and abundances of light elements Outline of stellar structure and evolution Neutron captur......actic chemical evolution : basic concepts and issues Some sp......fic GCE models and related observ......al data Origin and evolution of light elements......ology Chemical evolution in other sorts of galaxies Cosmic chemical evolution and diffuse backgr......me historical landmarks Appendix ...... Some physical and astronomical c......rbation theory and transition pro......5: Dissipation and abundance gradients Appendix ...
- 件名Galaxies -- Evolution. Cosmochemistry.
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- 要約等We summarize the oral and poster papers ......o observations of clusters of galaxies. Time constrai......etical aspects of cluster physic......for hard X-ray and soft WHIM emission, detection of clusters to th...... virial radius and scaling relations. Significan...
- 一般注記著者所属: Department of Physics, Tokyo......my, University of Hawaii
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- 要約等We present a Chandra analysis of the X-ray spectra of 56 clusters of galaxies at z>0.3, whic......perature range of 3>kT>15keV. Ou......rage, a factor of〜2 higher than ......s. We made use of combined spect...... as a function of redshift, but ......adii for a mix of cool-core and non cool-core ......by a power law of the form〜(1+z)....... The observed evolution implies that t......e iron content of the ICM at the......ch is a factor of〜2 larger than ......look-back time of 9Gyr. Our data......he time scales and physical proce......cal enrichment of the ICM.
- 一般注記...ory:Department of Physics and Astronomy, Johns Hopkins Univ...
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- 要約等...uclear outflow of the nearby sta......its morphology and to spectral va...... to the centre of the galaxy alo......t temperatures and the ionisation......the morphology of the outflow. W......y distribution of emission, show......to the nucleus and the disc. Limb brightening of the outflow, a......vations with Chandra and XMM-Newton, is...... between 550eV and 750eV.
- 一般注記...所属: Department of Physics & Astr......my, University of Leicester
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- 要約等...above the disk of the starburst ......ed with Suzaku and XMM-Newton. We...... Mg XI, Mg XII and the Fe-L compl......tal abundances of O, Ne, Mg, Si and Fe in this reg......ell with those of metal-poor stars and the model prediction of metals synthes......ent with those of type-Ia supern......hat the origin of the metals in ......als in the Cap and suggestion of the charge-exc...... the detection of hard X-ray emi......the north-east and north-west directions.
- 一般注記著者所属: Department of Physics, Kyoto University
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- 内容細目... : The Primary Structure that Sets Vert...... Is an Evasive Structure. 2. Well-defin......ared in animal evolution independently of the skeleton ;......ut vertebrates and the origin of the skeleton ; 4. Some of the most impor....... The Geometry of the Vertebrate......Takes the Form of Parallel Stripes and Concentric Cir......e the Products of Molecular Casc....... Longitudinal and transversal st......etric patterns of zebras and of transgenic mic......: the geometry of mammals become...... a main center of circularity wi......or development and evolution ; 9. The circularity of the vertebrate......eneral feature of vertebrates ; 11. Two poles o...
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- 要約等... K-shell lines of O and Mg were resolved clearly, and the abundances of O, Mg, Si, S and Fe were measur......in a 4' radius of NGC 1399 shows......lar abundances of Fe, Si and S, while the O/Fe and Mg/Fe abundanc...... about 0.4-0.5 and 0.7 in solar u......dii between 6' and 23', the Fe and Si abundances ...... 0.4-0.5 solar and show no signif......e ratios, O/Fe and Mg/Fe, are con......imately solar, and the O, Ne and Mg abundances ......ve enhancement of Fe within 130kpc of NGC 1399 and in NGC 1404 in......species O, Ne, and Mg which refle......t ratios for O and Fe within 130kpc of NGC 1399 are over an order of magnitude lower than those in...
- 一般注記著者所属: Department of Physics, Tokyo University of Science
紙図書
国立国会図書館
- 内容細目History and introduction The chemistry of organic matter......c compounds in galaxies Synthesis of organic compou......he late stages of stellar evolution Organic compou......ds as carriers of unsolved astro......omena Chemical structures of organic matter......ry simulations of molecular synthesis Origin of life on earth ...... from the past and outlook for th......mical infrared and submillimeter spectroscopic o...
紙図書
国立国会図書館
- 内容細目Stars and stellar evolution up to the Seco......War The legacy of the nineteenth......classification of stellar spectra Stellar structure and evolution The end points of stellar evolution The large-scale structure of the Universe 1......939 The Galaxy and the nature of the spiral neb......ae The origins of astrophysical ......The opening up of the electromag......The opening up of the electromagnetic spectrum and the new astron......e astrophysics of stars and galaxies since 1945 Stars and stellar evolution The physics of the interstell......um The physics of galaxies and clusters of galaxies High energy as...... determination of cosmological parameters The e...
- 一般注記...ted URL: Table of contents only http: //www.loc...
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- 内容細目...une : overview and perspectives /......ly development of ideas concerni...... B.G. Marsden, and C. VanLaerhoven The orbital and spatial distribution of the Kuiper bel......e distribution of multikilometer......lor properties and trends of the transneptu......et al.] Colors of Centaurs / S.C......ace properties of Kuiper belt objects and Centaurs from photometry and polarimetry / ......ic lightcurves of transneptunian objects and Centaurs : rot......tions, shapes, and densities / S.......d, P. Lacerda, and J.L. Ortiz Composition and surface properties of transneptunian objects and Centaurs / M.A......cal properties of Kuiper belt and Centaur objec...
- 一般注記Related URL: Table of contents only http: //www.loc...
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- 一般注記Includes bibliographical references (p. [295]-297) and index
- 並列タイトル等（連結）The structure & evolution of galaxies
- 並列タイトル等The structure & evolution of galaxies