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|a 9783319310060
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|a 3319310046
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|a 10.1007/978-3-319-31006-0
|2 doi
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|a (OCoLC)956646669
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|n Title purchased via APUC SHEDL / ScopNet ebook agreement
|n Physics and Astronomy (Springer-11651)
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|a QC1-999
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|a PG
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|a 530
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|a UAMI
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|a D'Onofrio, Mauro.
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|a From the Realm of the Nebulae to Populations of Galaxies :
|b Dialogues on a Century of Research.
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|a Cham :
|b Springer International Publishing,
|c 2016.
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|a 1 online resource (809 pages)
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|a text
|b txt
|2 rdacontent
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|a computer
|b c
|2 rdamedia
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|a online resource
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|a text file
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|b PDF
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|a Astrophysics and Space Science Library ;
|v v. 435
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|a Print version record.
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|a Foreword; Preface; Authors' Acknowledgments; Acronyms; Contents; List of Contributors; 1 Extragalactic Astronomy: From Pioneers to Big Science; 1.1 Outline of the Chapter; 1.2 The Pioneering Time; 1.3 From WWII to the Big Science: Some Geographic Angles; 1.3.1 USA: Preserving the Leadership; 1.3.1.1 The Progresses in Radio Astronomy; 1.3.2 The Extragalactic Research in the Ex Soviet Union; 1.3.3 UK and Commonwealth Countries; 1.3.4 The Dream of European Astronomers After WWII; 1.3.5 The Growth of Extragalactic Astronomy in Latin America; 1.3.6 The Japan Rush to Extragalactic Astronomy.
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|a 1.4 The Impact of New Detectors and Instruments1.5 Toward a Panchromatic View of Galaxies; 1.5.1 The Ultraviolet Window; 1.5.2 The Infrared Window; 1.5.3 The X-ray Window; 1.6 The Impact of Computing Power on Galaxy Modeling and Theoretical Understanding; 1.7 What Has Changed and What Is Changing in Galaxies Investigation?; 1.8 To Summarize; References; 2 The Milky Way and the Local Group; 2.1 Chapter Overview; 2.2 Milky Way: One of Many; 2.3 The Milky Way Dynamics and the Connection with Spirals; 2.3.1 Background; 2.3.2 Kapteyn's Universe; 2.3.3 Jan Hendrik Oort and Stellar Dynamics.
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|a 2.3.4 Properties and Evolution of the Velocity Ellipsoid2.3.5 Stellar Orbits; 2.3.6 Stability; 2.3.7 Determinations of Kinematic Properties; 2.3.8 Spiral Galaxies; 2.4 Milky Way: Stellar Population and the Interstellar Medium; 2.4.1 Early Revision of the Two Population Concept; 2.4.1.1 Towards a Galaxy Formation Picture; 2.4.2 Population II Complexity: The Discovery of the Thick Disk; 2.4.3 From Early Times to the Current View of the Milky Way; 2.4.3.1 Setting the Clocks: Age Determination; 2.4.3.2 Thin and Thick Disks, or the Disk?; 2.4.3.3 The Open Clusters as Disk Tracers; 2.4.3.4 The Halo.
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|a 2.4.3.5 The Globular Cluster Revolution2.4.3.6 The Bulge; 2.5 Milky Way: The Dust Component; 2.6 Beyond the Milky Way; 2.6.1 The Distance Scale Debate; 2.6.2 Primary Indicators; 2.6.2.1 Cepheids; 2.6.2.2 RR Lyrae Variables; 2.6.2.3 Tip of the Red Giant Branch Stars: The TRGB Method; 2.6.2.4 Advantages, Disadvantages and Caveats; 2.6.2.5 Crowding and Confusion; 2.6.3 Secondary Distance Indicators; 2.6.3.1 The Tully-Fisher Relation; 2.6.3.2 Type Ia Supernovæ; 2.7 The Companions of the Milky Way: The Local Group; 2.7.1 Andromeda; 2.7.2 The Dwarf Galaxy Population in the Local Group.
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|a 2.8 Tracing the Milky Way and the Local Group Co-evolution2.9 Just Outside the Local Group; 2.10 How Far Did We Go in Understanding the Milky Way and Nearby Universe; 2.11 To Summarize; References; 3 Family Traits of Galaxies: From the Tuning Fork to a Physical Classification in a Multi-Wavelength Context; 3.1 Chapter Overview; 3.2 The Varieties of Spiral Galaxies; 3.2.1 Discriminant Parameters in a Multi-Wavelength Context; 3.3 Filling the Abyss Between Ellipticals and Spirals: the S0 problem; 3.4 The Family of Early-Type Galaxies; 3.4.1 Learning from (Deep) Imaging the Outskirts of Galaxies.
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|a 3.4.2 The Depreciated Role of Mergers.
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|a In order to outline possible future directions in galaxy research, this book wants to be a short stopover, a moment of self-reflection of the past century of achievements in this area. Since the pioneering years of galaxy research in the early 20th century, the research on galaxies has seen a relentless advance directly connected to the parallel exponential growth of new technologies. Through a series of interviews with distinguished astronomers the editors provide a snapshot of the achievements obtained in understanding galaxies. While many initial questions about their nature have been addressed, many are still open and require new efforts to achieve a solution. The discussions may reveal paradigms worthwhile revisiting. With the help of some of those scientists who have contributed to it, the editors sketch the history of this scientific journey and ask them for inspirations for future directions of galaxy research.
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|a ProQuest Ebook Central
|b Ebook Central Academic Complete
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|a Physics.
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|a Astronomy
|v Observations.
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|a Astronomy
|x Observations.
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|a Astrophysics.
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|a Cosmology.
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|a Physics
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|a Physique.
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|a Astronomie
|v Observations.
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|a Astrophysique.
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|a Cosmologie.
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|a physics.
|2 aat
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|a astrophysics.
|2 aat
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|a cosmology.
|2 aat
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|a Astronomy
|2 fast
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|a Astrophysics
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|a Cosmology
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|a Physics
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|a Observations
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|a Rampazzo, Roberto.
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|a Zaggia, Simone.
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|i has work:
|a From the realm of the nebulae to populations of galaxies (Text)
|1 https://id.oclc.org/worldcat/entity/E39PCFGxm7GCRP84HtQbBbCBWC
|4 https://id.oclc.org/worldcat/ontology/hasWork
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776 |
0 |
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|i Print version:
|a D'Onofrio, Mauro.
|t From the Realm of the Nebulae to Populations of Galaxies : Dialogues on a Century of Research.
|d Cham : Springer International Publishing, ©2016
|z 9783319310046
|
830 |
|
0 |
|a Astrophysics and space science library.
|
856 |
4 |
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|u https://ebookcentral.uam.elogim.com/lib/uam-ebooks/detail.action?docID=4613374
|z Texto completo
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938 |
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|a ProQuest Ebook Central
|b EBLB
|n EBL4613374
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994 |
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|a 92
|b IZTAP
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