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
- 9 Galactic open clusters with supersolar metallicities
- 10 Old and very-metal-rich open clusters in the BOCCE project
- 11 Massive-star versus nebular abundances in the Orion nebula
- 12 Abundance surveys of metal-rich bulge stars
- 13 Metal abundances in the Galactic Center
- 14 Light elements in the Galactic bulge
- 15 Metallicity and ages of selected G–K giants
- Part III Observations – abundances in extragalactic contexts
- 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
11 - Massive-star versus nebular abundances in the Orion nebula
Published online by Cambridge University Press: 02 December 2009
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
- 9 Galactic open clusters with supersolar metallicities
- 10 Old and very-metal-rich open clusters in the BOCCE project
- 11 Massive-star versus nebular abundances in the Orion nebula
- 12 Abundance surveys of metal-rich bulge stars
- 13 Metal abundances in the Galactic Center
- 14 Light elements in the Galactic bulge
- 15 Metallicity and ages of selected G–K giants
- Part III Observations – abundances in extragalactic contexts
- 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 search for consistency between nebular and massive-star abundances has been a longstanding problem. I briefly review what has been done regarding this topic, also presenting a recent study focused on the Orion nebula: the O and Si stellar abundances resulting from a detailed and fully consistent spectroscopic analysis of the group of B stars associated with the Orion nebula are compared with the most recent nebular gas-phase results.
- Type
- Chapter
- Information
- The Metal-Rich Universe , pp. 94 - 99Publisher: Cambridge University PressPrint publication year: 2008
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