Article contents
Abundance study of two magnetic B-type stars in the Orion Nebula Cluster
Published online by Cambridge University Press: 23 January 2015
Abstract
We present the results of an abundance analysis of two magnetic B-type stars in the Orion Nebula Cluster that support the lack of a direct relationship between the existence of a magnetic field and a nitrogen excess in the photosphere.
- Type
- Contributed Papers
- Information
- Copyright
- Copyright © International Astronomical Union 2015
References
- 1
- Cited by