Hostname: page-component-78c5997874-g7gxr Total loading time: 0 Render date: 2024-11-13T09:36:31.336Z Has data issue: false hasContentIssue false

A Summary and Some Concluding Remarks

Published online by Cambridge University Press:  09 March 2010

V. V. Smith*
Affiliation:
National Optical Astronomy Observatory, 950 N. Cherry Ave. Tucson, AZ 85719USA email: vsmith@noao.edu
Rights & Permissions [Opens in a new window]

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

To present a summary of IAU Symposium 265 it is perhaps best to first step back and ask the question “Why did we meet in Rio to discuss chemical abundances?”. Part of the scientific rationale was to host a meeting that brought together researchers who probe chemical abundances and chemical evolution in all of the different astrophysical environments. All meetings should be planned such that they have an outcome and, with such a diverse set of abundance specialists brought together in one place to talk about their favorite topics, the stated outcome for IAUS265 was to provide, within our current understanding of the universe, a unified picture of the production of chemical elements over cosmic time; such a view is what I think of as cosmochemistry.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2010