Back to the Abstract


Article Contents
1 Introduction
2 Model atmospheres and line formation calculations
3 Spectral lines
4 The ATMOS infrared solar spectrum
5 CO line shapes and asymmetries
6 C and O isotopic abundance determinations
7 Comparisons with previous work
8 Conclusions
References
Online Material
Appendix A: ATMOS apodization
Appendix B: Scalefactors
Appendix C: Line lists

List of tables
List of figures

Copyright ESO 2006
Published by EDP Sciences