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Progress of Theoretical Physics Supplement No. 133



Gravitational Lensing and the High-Redshift Universe


Edited by Kenji Tomita and Toshifumi Futamase

Investigation on gravitational lensing phenomena and the evolution and spatial distribution of high-redshift objects occupies the most active part of various fields in cosmology and astrophysics. Gravitational lensing gives us many informations about the evolution and structure of galaxies and clusters, when we analyze multi-images of quasars and deformed images (such as arcs, arclets and rings) of galaxies caused by their lens objects, and brings also valuable informations about dark matter since gravitation feels the existence of invisible matter. Moreover they can amplify the luminosity of dark objects and play a role of a kind of telescopes. In recent years the microlensing phenomena due to stellar lens objects in Magellanic clouds and in the bulge in our Galaxy have been discovered and the successive observational and theoretical approaches to them have brought rapid progress in the studies on the structure of our Galaxy and the puzzling lens objects. On the other hand, the evolution and clustering of high-redshift objects have been clarified by recent observational studies of galaxies and clusters by optical, radio and X-ray telescopes and have led to wider and deeper understanding of galaxy formation theory.

This volume consists of nine review papers on the above topics, which were written by main talkers of the workshops (in 1997 and 1998) in Yukawa Institute for Theoretical Physics, based on their lectures and more recent research cotributions. It is therefore highly appropriate for students coming into cosmology and astrophysics, and also it gives good reviews of the present status and future prospects at a level accessible to the general researchers.


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