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010 a| 2013012345;

020 a| 9781107023802 (hard cover);

035 a| (WaSeSS)ssj0001036419;

042 a| pcc;

049 a| EREEa| NEHH;

050 00 a| QB858.8.L63b| C36 2008;

082 00 a| 523.1/122| 23;

111 2 a| Canary Islands Winter School of Astrophysicsn| (20th :d| 2008 :c| Tenerife, Canary Islands)?| UNAUTHORIZED;

245 10 a| Local Group cosmologyh| [electronic resource] /c| [edited by] David Martínez-Delgado, Max-Planck-Institut für Astronomie, Heidelberg.;

260 a| New York, NY :b| Cambridge University Press,c| 2013.;

300 a| xviii, 232 pages :a| illustrations ;c| 26 cm;

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

504 a| Includes bibliographical references.;

505 0 a| 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.;

506 a| Available only to authorized users.;

520 a| "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.;

538 a| Mode of access: World Wide Web;

651 0 a| Local Group (Astronomy)v| Congresses.=| ^A827222;

655 0 a| Electronic books.=| ^A491897;

700 1 a| Martínez Delgado, D.q| (David)?| UNAUTHORIZED;

856 40 z| Full text available from Ebook Central - Academic Completeu| https://ebookcentral.proquest.com/lib/eastcarolina/detail.action?docID=1394546;

949 a| CLICK ON WEB ADDRESSw| ASISh| JOYNER188;

949 a| CLICK ON WEB ADDRESSw| ASISh| HSL77;

949 a| CLICK ON WEB ADDRESSw| ASISh| JMUSIC60;

596 a| 1 3 4;

998 a| 5194875;

999 a| CLICK ON WEB ADDRESSw| ASISc| 1i| 5194875-1001l| JNETm| JOYNERr| Ys| Yt| JNESSBKu| 11/1/2019x| EBOOKz| JERESOURCE;

999 a| CLICK ON WEB ADDRESSw| ASISc| 1i| 5194875-2001l| HSLELECm| HSLr| Ys| Yt| HEBKu| 11/1/2019x| EBOOKz| HERESOURCE;

999 a| CLICK ON WEB ADDRESSw| ASISc| 1i| 5194875-3001l| MNETm| JMUSICr| Ys| Yt| MNESSBKu| 11/1/2019x| EBOOKz| JERESOURCE;

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

Author/creator	Canary Islands Winter School of Astrophysics
Other author	Martínez Delgado, D. (David)
Format	Electronic
Publication Info	New York, NY : Cambridge University Press, 2013.
Description	xviii, 232 pages : illustrations ; 26 cm
Supplemental Content	Full text available from Ebook Central - Academic Complete
Subjects	Local Group (Astronomy)--Congresses.

Contents	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.
Abstract	"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.
General note	Lectures presented at the XX Canary Islands Winter School of Astrophysics, held in Tenerife, Spain, November 17-18, 2008.
Bibliography note	Includes bibliographical references.
Access restriction	Available only to authorized users.
Technical details	Mode of access: World Wide Web
Genre/form	Electronic books.
LCCN	2013012345
ISBN	9781107023802 (hard cover)

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

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