Shy genel (9 risultati)

Lingua: Inglese
Editore: VDM Verlag Dr. Mueller Aktiengesellschaft & Co. KG, 2014
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Da: Books Puddle, New York, NY, U.S.A.Books Puddle
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Condizione: New. pp. 148.

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Da: preigu, Osnabrück, Germaniapreigu
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Taschenbuch. Condizione: Neu. The Formation of Dark Matter Halos and High-Redshift Galaxies | Shy Genel | Taschenbuch | 148 S. | Englisch | 2014 | LAP LAMBERT Academic Publishing | EAN 9783659382932 | Verantwortliche Person für die EU: preigu GmbH & Co. KG, Lengericher Landstr. 19, 49078 Osnabrück, mail[at]preigu[dot]de | Anbiet…er: preigu.

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Da: Mispah books, Redhill, SURRE, Regno UnitoMispah books
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Paperback. Condizione: Like New. LIKE NEW. SHIPS FROM MULTIPLE LOCATIONS. book.

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Da: BuchWeltWeit Ludwig Meier e.K., Bergisch Gladbach, GermaniaBuchWeltWeit Ludwig Meier e.K.
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Taschenbuch. Condizione: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -In the concordance cosmological model, galaxies form in the centers of dark matter halos and merge with one another following the mergers of their host halos. This book describes novel analysis methods, based on cosmological dark m…atter simulations, for quantifying the growth and merger rates of dark matter halos, and the surprising result that a significant fraction of the mass growth of dark matter halos may occur via a smooth component. Further, a modern description of observations and theories on the formation of massive star-forming galaxies about ten billion years ago is given. In particular, cosmological hydrodynamical simulations that model strong galactic winds are presented, and lessons on the evolution of massive star-forming regions in those galaxies are inferred. 148 pp. Englisch.

Lingua: Inglese
Editore: VDM Verlag Dr. Mueller Aktiengesellschaft & Co. KG, 2014
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Da: Majestic Books, Hounslow, Regno UnitoMajestic Books
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Condizione: New. Print on Demand pp. 148 2:B&W 6 x 9 in or 229 x 152 mm Perfect Bound on Creme w/Gloss Lam.

Lingua: Inglese
Editore: VDM Verlag Dr. Mueller Aktiengesellschaft & Co. KG, 2014
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Da: Biblios, frankfurt am main, HESSE, GermaniaBiblios
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EUR 61,60
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Condizione: New. PRINT ON DEMAND pp. 148.

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Da: moluna, Greven, Germaniamoluna
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Condizione: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Autor/Autorin: Genel ShyBorn in 1980 in Herzliya, Israel, Dr. Genel received his PhD in Astrophysics in 2011 at the Max-Planck-Institute for Extraterrestrial Physics near Munich, under the guidance of Professor Reinh…ard Genzel. He is currently an I.

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Da: buchversandmimpf2000, Emtmannsberg, BAYE, Germaniabuchversandmimpf2000
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Taschenbuch. Condizione: Neu. This item is printed on demand - Print on Demand Titel. Neuware -In the concordance cosmological model, galaxies form in the centers of dark matter halos and merge with one another following the mergers of their host halos. This book describes novel analysis methods, based on cosmological dark matte…r simulations, for quantifying the growth and merger rates of dark matter halos, and the surprising result that a significant fraction of the mass growth of dark matter halos may occur via a smooth component. Further, a modern description of observations and theories on the formation of massive star-forming galaxies about ten billion years ago is given. In particular, cosmological hydrodynamical simulations that model strong galactic winds are presented, and lessons on the evolution of massive star-forming regions in those galaxies are inferred.VDM Verlag, Dudweiler Landstraße 99, 66123 Saarbrücken 148 pp. Englisch.

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Da: AHA-BUCH GmbH, Einbeck, GermaniaAHA-BUCH GmbH
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EUR 61,19 spedizioneSpedito da Germania a U.S.A.Quantità: 1 disponibili
Taschenbuch. Condizione: Neu. nach der Bestellung gedruckt Neuware - Printed after ordering - In the concordance cosmological model, galaxies form in the centers of dark matter halos and merge with one another following the mergers of their host halos. This book describes novel analysis methods, based on cosmological dark matter… simulations, for quantifying the growth and merger rates of dark matter halos, and the surprising result that a significant fraction of the mass growth of dark matter halos may occur via a smooth component. Further, a modern description of observations and theories on the formation of massive star-forming galaxies about ten billion years ago is given. In particular, cosmological hydrodynamical simulations that model strong galactic winds are presented, and lessons on the evolution of massive star-forming regions in those galaxies are inferred.