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Buch, Englisch, Band 35, 344 Seiten, Format (B × H): 170 mm x 244 mm, Gewicht: 601 g
Reihe: Cambridge Astrophysics
Buch, Englisch, Band 35, 344 Seiten, Format (B × H): 170 mm x 244 mm, Gewicht: 601 g
Reihe: Cambridge Astrophysics
ISBN: 978-0-521-03743-3
Verlag: Cambridge University Press
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book examines the mass, stability and evolution of the Local Group as a whole and includes many important previously unpublished results and conclusions.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.
Autoren/Hrsg.
Fachgebiete
Weitere Infos & Material
Preface; 1. Introduction; 2. Local group membership; 3. The Andromeda galaxy (M31); 4. The Milky Way system; 5. The Triangulum galaxy (M33); 6. The Large Magellanic Cloud; 7. The Small Magellanic Cloud; 8. The elliptical galaxy M32 (= NGC 221); 9. The irregular dwarf galaxy NGC 6822; 10. The starburst galaxy IC 10; 11. Faint dwarf irregular galaxies; 12. Spheroidal galaxies; 13. The most luminous dwarf spheroidal galaxies; 14. Dwarf spheroidals in the Andromeda subgroup; 15. Faint dwarf spheroidals; 16. The outer fringes of the Local Group; 17. Intergalactic matter in the Local Group; 18. Dynamical and physical evolution; 19. Properties of the Local Group; 20. Conclusions; Glossary; Bibliography; Object index.
