Galaxy evolution across the Hubble time : proceedings of the 235th Symposium of the International Astronomical Union held in Prague, Czech Republic, August 14-17, 2006
著者
書誌事項
Galaxy evolution across the Hubble time : proceedings of the 235th Symposium of the International Astronomical Union held in Prague, Czech Republic, August 14-17, 2006
（IAU symposium and colloquium proceedings series, . IAU Symposium ; no. 235）
Cambridge University Press, 2007
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注記
Includs bibliographical refarences and indexies
内容説明・目次
内容説明
This last decade has witnessed a revolution in our observations of galaxies; in particular deep imaging with HST and spectroscopy with 10m-class ground-based telescopes have uncovered many objects that are difficult to place along the Hubble sequence. High resolution spectroscopy of extremely faint objects has enabled the study of the kinematic evolution and, hence, the mass assembly of galaxies to unprecedented look-back times for direct comparison with cosmological structure formation scenarios. Thus, it is now possible to study all three aspects of galaxy evolution - their morphological-dynamical, chemical and spectral evolution out to redshift larger than six, exploring more than 95% of the age of the universe. These Proceedings of the IAU Symposium 235 report the considerable progress made in recent years on galaxy formation and evolution, and look forward to the expected breakthroughs in the domain of remote galaxies, with ALMA, the ELT and the next generation space telescopes.
目次
- Preface
- 1. Galaxy building blocks
- 2. Environment and interactions
- 3. Star formation processes and feedback
- 4. The early Universe
- Author index.
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