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One of the most fascinating unresolved problems of modern astrophysics is how the galaxies we observe today were formed. The Lambda-Cold Dark Matter paradigm predicts that large spiral galaxies such as the Milky Way formed through accretion and tidal disruption of satellite galaxies. The galaxies of the Local Group provide the best laboratory in which to investigate these galaxy formation processes because they can be studied with sufficiently high resolution to exhume fossils of galactic evolution embedded in the spatial distribution, kinematics, and chemical abundances of their oldest stars. Based on the twentieth Winter School of the Canary Islands Institute of Astrophysics, this volume provides a firm grounding for graduate students and early career researchers working on Local Group cosmology. It presents modules from eight eminent and experienced scientists at the forefront of Local Group research, and includes overviews of observational techniques, diagnostic tools, and various theoretical models.
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The Local Group is a small cluster of galaxies that includes the Milky Way. At least half of all galaxies in the Universe are thought to belong to similar groups. This authoritative volume provides a comprehensive synthesis of what is known about the Local Group. It begins with a summary of each member galaxy, as well as those galaxies previously regarded as possible members. The book examines the mass, stability and evolution of the Local Group as a whole and includes many important previously unpublished results and conclusions. With clarity, Professor van den Bergh provides a masterful summary of all that is known about the galaxies of the Local Group and their evolution, and expertly places this knowledge in the wider context of on-going studies of galaxy formation and evolution, the cosmic distance scale, and the conditions in the early Universe.
Local Group (Astronomy) --- Local Group (Astronomy). --- Local Group of galaxies
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Studies of Nearby Galaxies are currently the focus of many observations and numerical simulations. This book presents an overview of the galaxies within the Local Volume (D < 10 Mpc), including the Local Group (D < 1 Mpc) and our closest neighbours, the Andromeda Galaxy and the Magellanic Clouds. Presented are the latest results from radio, infrared and optical surveys as well as detailed multi-wavelength studies of individual galaxies. Accurate distances are now available for the majority of Local Volume galaxies providing a true 3-dimensional view of their distribution and flow pattern as well as their star formation.
Physics. --- Astronomy, Astrophysics and Cosmology. --- Astronomy. --- Astrophysics. --- Physique --- Astronomie --- Astrophysique --- Andromeda Galaxy -- Congresses. --- Interstellar matter -- Congresses. --- Local Group (Astronomy) -- Congresses. --- Triangulum Galaxy -- Congresses. --- Astronomy & Astrophysics --- Physical Sciences & Mathematics --- Astrophysics --- Galaxies --- Local Group (Astronomy) --- Local Group of galaxies --- Cosmology. --- Observations, Astronomical. --- Astronomy --- Space sciences. --- Astrophysics and Astroparticles. --- Extraterrestrial Physics, Space Sciences. --- Astronomy, Observations and Techniques. --- Observations. --- Space Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics). --- Astronomical physics --- Cosmic physics --- Physics --- Astronomy—Observations. --- Astronomical observations --- Observations, Astronomical --- Science and space --- Space research --- Cosmology --- Science
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