Local Group cosmology /edited by] David Martínez-Delgado, Max-Planck-Institut für Astronomie, Heidelberg.

Contributor(s):

Material type: Text

text

Media type:

computer

Carrier type:

online resource

ISBN:

9781107416567

Genre/Form:

Electronic Books.

LOC classification:

QB858 .L633 2013

Online resources:

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Available additional physical forms:

Contents:

K.C. Freeman -- Dark matter content and tidal effects in Local Group dwarf galaxies / Steven R. Majewski -- Notes on the missing satellites problem / James Bullock -- The Milky Way satellite galaxies -- Stellar tidal streams / R. Ibata -- Tutorial : the analysis of colour-magnitude diagrams / D. Valls-Gabaud -- Tutorial : modelling tidal streams using n-body simulations / J. Peñarrubia.

Subject: "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, a notion previously postulated on empirical grounds from the character of stellar populations found in our Galaxy. The Local Group galaxies are 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"--Provided by publisher.

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Holdings
Item type	Current library	Collection	Call number	URL	Status	Date due	Barcode
Online Book (LOGIN USING YOUR MY CIU LOGIN AND PASSWORD)	G. Allen Fleece Library ONLINE	Non-fiction	QB858.8.63 (Browse shelf(Opens below))	Link to resource	Available		ocn864552413

Lectures presented at the XX Canary Islands Winter School of Astrophysics, held in Tenerife, Spain, November 17-18, 2008.

"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, a notion previously postulated on empirical grounds from the character of stellar populations found in our Galaxy. The Local Group galaxies are 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"--Provided by publisher.

Includes bibliographical references.

The formation of the Milky Way in the CDM paradigm / K.C. Freeman -- Dark matter content and tidal effects in Local Group dwarf galaxies / Steven R. Majewski -- Notes on the missing satellites problem / James Bullock -- The Milky Way satellite galaxies -- Stellar tidal streams / R. Ibata -- Tutorial : the analysis of colour-magnitude diagrams / D. Valls-Gabaud -- Tutorial : modelling tidal streams using n-body simulations / J. Peñarrubia.

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