Cantitate/Preț
Produs

Galaxies in the Young Universe: Proceedings of a Workshop Held at Ringberg Castle, Tegernsee Germany, 22–28 September 1994.: Lecture Notes in Physics, cartea 463

Editat de Hans Hippelein, Klaus Meisenheimer, Hermann-Josef Röser
en Limba Engleză Paperback – 17 apr 2014
Understanding the formation and evolution of early galaxies is one of the most challenging problems in modern astronomy. In this volume leading specialists describe observations of high and intermediate redshift galaxies as well as the deep survey activities. Further topics include cosmology, and modelling and computer simulations of galaxy formation. Thus the reader will find here a fairly complete picture of the state of the art in this active field of astrophysics research.
Citește tot Restrânge

Din seria Lecture Notes in Physics

Preț: 63154 lei

Preț vechi: 74299 lei
-15% Nou

Puncte Express: 947

Preț estimativ în valută:
12086 12591$ 10049£

Carte tipărită la comandă

Livrare economică 08-22 februarie 25

Preluare comenzi: 021 569.72.76

Specificații

ISBN-13: 9783662140222
ISBN-10: 3662140225
Pagini: 336
Ilustrații: XV, 317 p. 34 illus., 4 illus. in color.
Dimensiuni: 155 x 235 x 18 mm
Greutate: 0.47 kg
Ediția:Softcover reprint of the original 1st ed. 1995
Editura: Springer Berlin, Heidelberg
Colecția Springer
Seria Lecture Notes in Physics

Locul publicării:Berlin, Heidelberg, Germany

Public țintă

Research

Cuprins

The hot big bang and beyond.- Cosmological structure formation in hot and cold dark matter scenarios.- Observations and cosmological models.- Fluctuation spectra and high-redshift objects.- Galaxies at high redshift: 1994.- High-redshift Milli-Jansky radio galaxies.- Spectroscopy and imaging of a forming galaxy causing damped ly ? absorption at z=2.81.- Ly ? absorption in 4C 41.17.- The revolution in studies of distant radio galaxies.- Detection of 10h ?1 Mpc quasar/absorber correlation at high redshift.- Large-scale structure at z?2.5.- Spectroscopy of 600 faint field galaxies at CFHT: luminosity function to z=1 and properties of blue emission-line galaxies at z