Book contents
- Frontmatter
- Contents
- List of contributors
- Preface
- Part I Abundances in the Galaxy: field stars
- Part II Abundances in the Galaxy: Galactic stars in clusters, bulges and the centre
- Part III Observations – abundances in extragalactic contexts
- 16 Stellar abundances of early-type galaxies
- 17 Measuring chemical abundances in extragalactic metal-rich H ii regions
- 18 On the maximum oxygen abundance in metal-rich spiral galaxies
- 19 Starbursts and their contribution to metal enrichment
- 20 High metallicities at high redshifts
- 21 Evolution of dust and elemental abundances in quasar DLAs and GRB afterglows as a function of cosmic time
- 22 Dust, metals and diffuse interstellar bands in damped Lyman-alpha systems
- 23 Tracing metallicities in the Universe with the James Webb Space Telescope
- Part IV Stellar populations and mass functions
- Part V Physical processes at high metallicity
- Part VI Formation and evolution of metal-rich stars and stellar yields
- Part VII Chemical and photometric evolution beyond Solar metallicity
23 - Tracing metallicities in the Universe with the James Webb Space Telescope
Published online by Cambridge University Press: 02 December 2009
- Frontmatter
- Contents
- List of contributors
- Preface
- Part I Abundances in the Galaxy: field stars
- Part II Abundances in the Galaxy: Galactic stars in clusters, bulges and the centre
- Part III Observations – abundances in extragalactic contexts
- 16 Stellar abundances of early-type galaxies
- 17 Measuring chemical abundances in extragalactic metal-rich H ii regions
- 18 On the maximum oxygen abundance in metal-rich spiral galaxies
- 19 Starbursts and their contribution to metal enrichment
- 20 High metallicities at high redshifts
- 21 Evolution of dust and elemental abundances in quasar DLAs and GRB afterglows as a function of cosmic time
- 22 Dust, metals and diffuse interstellar bands in damped Lyman-alpha systems
- 23 Tracing metallicities in the Universe with the James Webb Space Telescope
- Part IV Stellar populations and mass functions
- Part V Physical processes at high metallicity
- Part VI Formation and evolution of metal-rich stars and stellar yields
- Part VII Chemical and photometric evolution beyond Solar metallicity
Summary
The James Webb Space Telescope is a 6.6-m-aperture, passively cooled space observatory optimized for near-IR observations. It will be one of the most important observing facilities in the next decade, and it is designed to address numerous outstanding issues in astronomy. In this article we focus specifically on its capabilities to investigate the chemical abundances of various classes of astronomical objects and their metallicity evolution through the cosmic epochs.
- Type
- Chapter
- Information
- The Metal-Rich Universe , pp. 212 - 224Publisher: Cambridge University PressPrint publication year: 2008