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Galaxies in the Local Volume de Bärbel Silvia Koribalski

Galaxies in the Local Volume: Astrophysics and Space Science Proceedings

Editat de Bärbel Silvia Koribalski, H. Jerjen
en Limba Engleză Paperback – 10 oct 2011
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.
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Specificații

ISBN-13: 9789048177691
ISBN-10: 9048177693
Pagini: 380
Ilustrații: XX, 360 p.
Dimensiuni: 155 x 235 x 21 mm
Greutate: 0.58 kg
Ediția:2008
Editura: Springer
Colecția Astrophysics and Space Science Proceedings
Seria Astrophysics and Space Science Proceedings

Locul publicării:Dordrecht, Netherlands

Public țintă

Research

Cuprins

Invited and Contributed Talks.- Poster Contributions.

Notă biografică

B.S. Koribalski (Physics Diploma and PhD from the University of Bonn, Germany; now Senior Research Scientist at the CSIRO Australia Telescope National Facility; PI of the "Local Volume HI Survey" (LVHIS), etc.)

Textul de pe ultima copertă

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.

Caracteristici

Provides a timely review on the subject of the Local Volume given the many recent advances on this topic Combines observations, simulations and theoretical developments The conference was attended by top scientists in the field