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Abundance study of two magnetic B-type stars in the Orion Nebula Cluster

Published online by Cambridge University Press:  23 January 2015

T. Morel
T. Morel*
Affiliation:
Institut d'Astrophysique et de Géophysique, Allée du 6 Août, 4000 Liège, Belgium email: morel@astro.ulg.ac.be
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Abstract

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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
Proceedings of the International Astronomical Union , Volume 9 , Issue S307: New windows on massive stars: asteroseismology, interferometry, and spectropolarimetry , June 2014 , pp. 451 - 452
Copyright
Copyright © International Astronomical Union 2015 

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