Fig. 2 from Pristine CNO Abundances from Magellanic Cloud B Stars. II. Fast Rotators in the Large Magellanic Cloud Cluster NGC 2004

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Pristine CNO Abundances from Magellanic Cloud B Stars. II. Fast Rotators in the Large Magellanic Cloud Cluster NGC 2004

Authors: A. J. Korn, M. F. Nieva, S. Daflon, and K. Cunha

Korn et al. 2005 The Astrophysical Journal 633 899.

Provider: AAS Journals

Caption: Fig. 2.

Example of how the Hγ profile constrains the stellar parameters. The main dependencies are T_eff and ﹩\mathrm{log}\,g﹩; [M/Fe] and ﹩v\mathrm{sin}\,i﹩ play a minor role (not shown here).

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